cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Dataverse. GRO.data - Schulung im Forschungsdatenmanagement (UB Hildesheim).
Creators: name: Strauch, Annette
Publisher: name: Zenodo
Year: 2021
Subjects: FDM
Dataverse
Data Publication
Forschungsdatenveröffentlichung
UB Hildesheim
RDM
Bibliotheken
Universitätsbibliotheken

description: GRO.data ist das universelle Forschungsdatenrepositorium für Forscherinnen und Forscher an den Universitäten in Niedersachsen, um Forschungsdaten zu publizieren. Dieser Service wird von der GWDG gehostet, die sich um Datensicherheit und -schutz, einschließlich Backups und Zugriffskontrolle sowie um die Verfügbarkeit und Zuverlässigkeit, kümmert. Das Dataverse-Projekt wird am Harvard- Institut für quantitative Sozialwissenschaften(IQSS) zusammen mit vielen Mitwirkenden weltweit entwickelt. Datensätze können so auf einfache Art dauerhaft gesichert und Änderungen an Datensätzen über mehrere Versionen hinweg verfolgt werden. Forschungsdaten können außerdem hier geteilt und öffentlich verfügbar gemacht werden (Datenpublikationen mit persistenten Identifikatoren). Wenn Sie eine ORCID iD haben, können Ihre Daten auch automatisch zu Ihrem ORCID record hinzugefügt werden. GRO.data wird weiterhin kontinuierlich von der Göttinger eResearch Alliance angepasst. Wenn wir fachspezifische Repositorien für die Disziplin kennen, empfehlen wir immer zuerst die Forschungsdaten in den disziplinspezifischen Repositorien hochzuladen (re3data; https://www.re3data.org/browse/). Auch jede Forscherin und jeder Forscher der Stiftung Universität Hildesheim kann ihr/sein institutionelles Konto nutzen (‘Log-In’ über die Academic Cloud: https://academiccloud.de/) und ein persönliches „Dataverse“ anlegen, um Forschungsdaten als „Datasets“ hochzuladen. Wichtige Themen: * Datenupload * Metadatenschemata * Daten im Portal bearbeiten * Daten veröffentlichen (Data Publication) Service-URL: https://data.goettingen-research-online.de/ 
title: Ð¤Ð¸Ð·Ð¸ÐºÐ¾-ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð²Ð¾Ð»Ð½Ð¾Ð²ÑÑ Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð² Ð² MOEMS ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°Ñ
title: ÑÑÐµÐ±Ð½Ð¸Ðº Ð¿ÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² 16.04.01 Â«Ð¢ÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â»
titleType: Subtitle
Creators: name: ÐÑÑÐ¸Ð¿Ð¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
name: ÐÐ»Ð°Ð´ÐºÐ¸Ð¹, ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹
name: ÐÑÑÑÐºÐ¾, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ¸ÑÑÑÐ¸Ð½, Ð¡ÐµÑÐ³ÐµÐ¹
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: Ð¤Ð¾ÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÑÐ¸Ð±Ð¾ÑÑ
ÐÐ¿ÑÐ¸ÐºÐ¾-ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÑÐ¸Ð±Ð¾ÑÑ

description: Ð£ÑÐµÐ±Ð½Ð¸Ðº Ð½Ð°Ð¿Ð¸ÑÐ°Ð½ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð»ÐµÐºÑÐ¸Ð¹ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¼Ð¸ÐºÑÐ¾- Ð¸ ÑÐ°Ð´Ð¸Ð¾ÑÐ¾ÑÐ¾Ð½Ð¸ÐºÐ¸Â», ÐºÐ¾ÑÐ¾ÑÑÐµ Ð°Ð²ÑÐ¾ÑÑ ÑÐ¸ÑÐ°ÑÑ Ð½Ð° Ð¿ÑÐ¾ÑÑÐ¶ÐµÐ½Ð¸Ð¸ ÑÑÐ´Ð° Ð»ÐµÑ Ð½Ð° ÑÐ°ÐºÑÐ»ÑÑÐµÑÐµ ÑÐ°Ð´Ð¸Ð¾ÑÐµÑÐ½Ð¸ÐºÐ¸ Ð¸ ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²-Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Â«Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â», Â«Ð¤Ð¾ÑÐ¾Ð½Ð¸ÐºÐ°Â», Â«ÐÐ¿ÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐ°Â». ÐÐ·Ð»Ð¾Ð¶ÐµÐ½ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð», Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐ¹ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÑÐ¾Ð¹ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ, Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¿Ð»Ð°Ð½, Ð¿ÑÐ¸Ð¼ÐµÑÐ½ÑÐ¹ ÑÐ¿Ð¸ÑÐ¾Ðº Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð´Ð»Ñ ÑÐºÐ·Ð°Ð¼ÐµÐ½Ð°.
Ð ÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ â Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°Ð¼ Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°Ð¼, ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ°Ð¼ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â», Â«Ð¤Ð¾ÑÐ¾Ð½Ð¸ÐºÐ°Â» Ð¸ Â«ÐÐ¿ÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐ°Â», Ð° ÑÐ°ÐºÐ¶Ðµ Ð»Ð¸ÑÐ°Ð¼, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¸Ð½ÑÐµÑÐµÑÑÑÑÑÑ Ð½Ð¾Ð²ÑÐ¼Ð¸ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°Ð¼Ð¸ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐ¼Ð¸, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÐ¼Ð¸ Ð² Ð¼Ð¸ÐºÑÐ¾Ð¼Ð¸ÑÐµ.
Radio emission and jets from microquasars
Creators: name: Gallo, E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: To some extent, all Galactic binary systems hosting a compact object are potential `microquasars', so much as all galactic nuclei may have been quasars, once upon a time. The necessary ingredients for a compact object of stellar mass to qualify as a microquasar seem to be: accretion, rotation and magnetic field. The presence of a black hole may help, but is not strictly required, since neutron star X-ray binaries and dwarf novae can be powerful jet sources as well. The above issues are broadly discussed throughout this Chapter, with a a rather trivial question in mind: why do we care? In other words: are jets a negligible phenomenon in terms of accretion power, or do they contribute significantly to dissipating gravitational potential energy? How do they influence their surroundings? The latter point is especially relevant in a broader context, as there is mounting evidence that outflows powered by super-massive black holes in external galaxies may play a crucial role in regulating the evolution of cosmic structures. Microquasars can also be thought of as a form of quasars for the impatient: what makes them appealing, despite their low number statistics with respect to quasars, are the fast variability time-scales. In the first approximation, the physics of the jet-accretion coupling in the innermost regions should be set by the mass/size of the accretor: stellar mass objects vary on 10^5-10^8 times shorter time-scales, making it possible to study variable accretion modes and related ejection phenomena over average Ph.D. time-scales. [Abridged]
description: 28 pages, 13 figures, To appear in Belloni, T. (ed.): The Jet Paradigm - From Microquasars to Quasars, Lect. Notes Phys. 794 (2009)
Optical, ultraviolet, and infrared observations of isolated neutron stars
Creators: name: Mignani, Roberto P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Forty years passed since the optical identification of the first isolated neutron star (INS), the Crab pulsar. 25 INSs have been now identified in the optical (O), near-ultraviolet (nUV), or near-infrared (nIR), hereafter UVOIR, including rotation-powered pulsars (RPPs), magnetars, and X-ray-dim INSs (XDINSs), while deep investigations have been carried out for compact central objects (CCOs), Rotating RAdio transients (RRATs), and high-magnetic field radio pulsars (HBRPs). In this review I describe the status of UVOIR observations of INSs, their emission properties, and I present the results from recent observations.
description: 25 pages, 8 figures, accepted for publication in Advances in Space Research
Risk factors of septic shock development and thirty-day mortality with a predictive model in adult candidemia patients in intensive care units
Creators: name: Suh, Jin Woong
name: Kim, Min Ja
name: Kim, Jong Hun
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: This study aimed to investigate factors associated with septic shock development and 30-day mortality outcome with a prediction model among adult candidemia patients in the intensive care unit (ICU). A retrospective study was conducted among patients admitted to the ICU from 2009 to 2018 at a tertiary care medical centre. The study subjects included adult patients ≥ 19 years with candidemia treated with antifungal agent for ≥ 3 days. Clinical variables were collected and analysed. A total of 126 patients were included in the study. Of these patients, 32 patients (25.4%) had septic shock. Multivariate logistic regression analysis revealed that chronic liver disease was associated with septic shock (odds ratio [OR] 3.372, 95% confidence interval [CI] 1.057 − 10.057). The rate of 30-day mortality was 35.7% and the associated mortality risk factors were malignancy (OR 8.251, 95% CI 2.227 − 30.573), chronic liver disease (OR 3.605, 95% CI 0.913 − 14.227), haemodialysis (OR 8.479, 95% CI 1.801 − 39.924), mycological failure (OR 29.675, 95% CI 7.012 − 125.578), and septic shock (OR 3.980, 95% CI 1.238 − 12.796). A predictive model for 30-day mortality was created based on the mortality risk factor scores, which had an area of 0.862 under the receiver operating characteristic curve. Adult candidemia patients in the ICU who have chronic liver disease may be at higher risk of developing septic shock. Furthermore, our predictive model for 30-day mortality based on the mortality risk factors may be useful for clinical assessment.
Lycogala epidendrum L.) Fr
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Cribrariales
Tubiferaceae
Lycogala
Lycogala epidendrum

description: Lycogala epidendrum (aggr.) (L.) Fr.,
koksnes vilkpienaine
- leg.&det. W.Rotert, 1890; (JK), very common. Given the fact that the genus Lycogala is currently being revised and several new species have been and will be described, it has been decided in this paper to treat L. epidendrum as a species complex.
description: Published as part of Kluša, Julita, 2023, Complete Checklist Of Myxomycetes In Latvia, pp. 127-151 in Acta Biologica Universitatis Daugavpiliensis 23 (2) on pages 127-151, DOI: 10.59893/abud.23(2).002, http://zenodo.org/record/12650118
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼Ð¾Ð½Ð¸ÑÐ¾ÑÐ¸Ð½Ð³Ð° Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð³Ð¾ Ð±Ð°Ð½ÐºÐ° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ°Ð½Ðº Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Â»
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ½, ÐÑÐ»Ð¸Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÑÑ
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼Ð¾Ð½Ð¸ÑÐ¾ÑÐ¸Ð½Ð³Ð°
Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ
Ð°Ð½Ð°Ð»Ð¸Ð· Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ°Ð½Ðº Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Â».
ÐÐµÑÐ¾Ð´Ð°Ð¼Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Ð¿Ð¾ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÐ¼Ðµ, Ð¾Ð±Ð¾Ð±ÑÐµÐ½Ð¸Ðµ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð°Ð½Ð°Ð»Ð¸Ð·Ð°, ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ, Ð´ÐµÐ´ÑÐºÑÐ¸Ð¸, Ð¸Ð½Ð´ÑÐºÑÐ¸Ð¸, ÑÐ¸Ð½ÑÐµÐ·Ð°.
Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ â Ð¿Ð¾Ð¸ÑÐº Ð¿ÑÑÐµÐ¹ Ð´Ð»Ñ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð³Ð¾ Ð±Ð°Ð½ÐºÐ°. ÐÑÐ½Ð¾Ð²Ð½ÑÐ¼Ð¸ Ð·Ð°Ð´Ð°ÑÐ°Ð¼Ð¸ ÑÐ²Ð»ÑÐ»Ð¸ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÐ½Ð¾ÑÑÐ¸ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð³Ð¾ Ð±Ð°Ð½ÐºÐ°; ÑÐ°ÐºÑÐ¾ÑÑ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÐ¸Ðµ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð³Ð¾ Ð±Ð°Ð½ÐºÐ°, Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð², ÑÐµÐ»Ð¸, Ð·Ð°Ð´Ð°Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð³Ð¾ Ð±Ð°Ð½ÐºÐ°; ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¸ Ð½Ð°Ð´Ð·Ð¾ÑÐ° Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð³Ð¾ Ð±Ð°Ð½ÐºÐ°, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ ÐÐÐÂ Â«ÐÐ°Ð½Ðº Â«Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Â».
Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÑÑ.
Ð¢Ð°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÐ¾Ð²Ð½Ñ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ Ð±Ð°Ð»Ð°Ð½ÑÐ° ÐÐÐÂ Â«ÐÐ°Ð½Ðº Â«Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Â», ÑÑÐ¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÑÑ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ.
Gauge-Higgs Unification: Stable Higgs Bosons as Cold Dark Matter
Creators: name: Hosotani, Yutaka
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the gauge-Higgs unification the 4D Higgs field becomes a part of the extra-dimensional component of the gauge potentials. In the $SO(5) \times U(1)$ gauge-Higgs unification in the Randall-Sundrum warped spacetime the electroweak symmetry is dynamically broken through the Hosotani mechanism. The Higgs bosons become absolutely stable, and become the dark matter of the universe. The mass of the Higgs boson is determined from the WMAP data to be about 70 GeV.
description: 14 pages, 5 figures. Proceeding for SCGT09.
Higher rate of SARS-CoV-2 IgG seropositivity in hospital-based healthcare workers compared to elderly care staff in a Swedish low-prevalence region: a cross-sectional study
Creators: name: Ocias, Lukas Frans
name: Skogstam, Anna
name: Kjerstadius, Torbjörn
name: Lundin, Fredrik
name: Tevell, Staffan
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Previous seroprevalence studies have demonstrated higher anti-SARS-CoV-2 IgG seroprevalence in healthcare workers (HCWs) than in the background population during the first phase of the 2020 COVID-19 pandemic. These studies, however, focussed mainly on hospital employees. To perform a cross-sectional study comparing the seroprevalence of hospital-based HCWs with those employed in elderly care (home care and nursing homes). Employees (n = 4955) in the county of Värmland, Sweden, were recruited between weeks 27 and 42 and tested for IgG antibodies against SARS-CoV-2. Serological results were combined with self-reported questionnaire data. IgG seroprevalence was 5.7% in the total group of HCWs, and was higher among those employed in hospital-based healthcare than among those working in elderly care (8.4% vs. 3.7%, p The difference in seroprevalence between HCWs in the two settings suggests that not only the profession but also factors in the workplace environment may be of importance. As all studied exposures were associated with IgG seropositivity, and asymptomatic infection was detected in 7.5% of participants, preventing outbreaks among HCWs is challenging. Adequate use of personal protective equipment when working with patients regardless of COVID-19 status, source control in situations with co-workers in which distancing is not possible, and routines enabling symptomatic staff to isolate pending PCR results are required to prevent healthcare-associated outbreaks of COVID-19.
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¼Ð¾Ð»Ð¾Ð´ÐµÐ¶Ð½Ð¾Ð³Ð¾ ÐºÐ°ÑÐµ Ð½Ð° 50 Ð¼ÐµÑÑ Ð² ÐÑÐ±Ð¾ÑÐ³ÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÑÐµÐ²Ð°, ÐÐºÑÐ°Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¼Ð¾Ð»Ð¾Ð´ÐµÐ¶Ð½Ð¾Ðµ ÐºÐ°ÑÐµ
ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ
ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ñ
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÐµÐ¼
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÑÑÑ Ð¿ÑÐ¾ÐµÐºÑ Ð¼Ð¾Ð»Ð¾Ð´ÐµÐ¶Ð½Ð¾Ð³Ð¾ ÐºÐ°ÑÐµ Ð½Ð° 50 Ð¿Ð¾ÑÐ°Ð´Ð¾ÑÐ½ÑÑ Ð¼ÐµÑÑ Ð² ÐÑÐ±Ð¾ÑÐ³ÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ.
 ÐÑÐ»Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð° ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ñ ÐºÐ°ÑÐµ, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿Ð»Ð¾ÑÐ°Ð´Ñ Ð¼Ð¾Ð»Ð¾Ð´ÐµÐ¶Ð½Ð¾Ð³Ð¾ ÐºÐ°ÑÐµ. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð´Ð¾Ð»Ð¶Ð½Ð¾ÑÑÐ½Ð°Ñ Ð¸Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð±Ð°ÑÐ¼ÐµÐ½Ð°; ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸, Ð¾Ð±ÑÑÐ»Ð°Ð²Ð»Ð¸Ð²Ð°ÑÑÐ¸Ðµ ÑÐµÑÑÑÑÐ½ÑÐ¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð» Ð¸ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÑ Ð¾ÑÐºÑÑÑÐ¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
ÐÐ»ÑÑÐµÐ²ÑÐµ ÑÐ»Ð¾Ð²Ð°: Ð¼Ð¾Ð»Ð¾Ð´ÐµÐ¶Ð½Ð¾Ðµ ÐºÐ°ÑÐµ, ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ, ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ñ, Ð¼ÐµÐ½Ñ, ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÐµÐ¼, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ.
Behaviour and movement of return migrating adult Chinook salmon (Oncorhynchus tshawytscha) through the Salish Sea
Creators: name: Hendriks, Brian James Lambert
Publisher: name: University of British Columbia
Year: 2024

description: I used acoustic tags with depth sensors and a series of sentinel underwater acoustic receiver arrays to track adult Chinook salmon (Oncorhynchus tshawytscha) through the southern Salish Sea towards their natal rivers. My objectives were to: i) identify areas and routes most utilized by migrating salmon, ii) determine travel times and rates between areas, and iii) identify depth distributions exhibited by migrating Chinook salmon. I tagged 114 adult Chinook salmon, from 14 different river systems, nearshore to Port Renfrew, BC during the summers of 2019 and 2020. Based on migration path criteria, 35 individuals took direct routes towards natal rivers, 35 individuals took non-direct routes, and 44 could not be categorized. Only Fraser River fish consistently took direct paths towards their natal river. Tagged fish were largely detected in the surface waters between 0-30 m (mean 22.0 m) throughout all areas of study, rarely detected below 100 m, and were orientated primarily nearshore. Average migration rates varied among stocks from 0.25 BL/s to 0.65 BL/s (0.84 to 2.02 km/h). There were no effects of somatic energy index, sex, or year on these rates. Fraser River Chinook slowed as they approached their natal river, with an average migration rate 3 times faster in Juan de Fuca Strait (0.66 BL/s; 2.09 km/h) compared to the Fraser estuary (0.22 BL/s; 0.67 km/h). Fraser River Chinook salmon are significant prey to Southern Resident Killer Whales (SRKW; Orcinus orca) but did not seem to exhibit any different behaviours in terms of migration rates or depth patterns through known SRKW feeding regions relative to other areas. The survival of tagged Fraser River fish was relatively high through all segments. The fact that Fraser fish migrated at some of the fastest rates observed might indicate some form of anti-predator behaviour. Alternatively, these fast migration rates may reflect an urgency to reach the Fraser River and initiate arduous freshwater migration prior to spawning. This study is the first to describe migration behaviours of several stocks of adult Chinook salmon during their homeward marine migrations by providing detailed insights into migration routes, rates, and depths.
title: ÐÐ»Ð¸ÑÐ½Ð¸Ðµ Ð¼Ð°ÐºÑÐ¾ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð½Ð° ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¾Ð½Ð´Ð¾Ð²Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¡Ð¨Ð)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¾ÐºÐ¾ÑÑÐµÐ², ÐÐ¸ÑÐ¸Ð»Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð±ÐµÐ·ÑÐ°Ð±Ð¾ÑÐ¸ÑÐ°
Ð¸Ð½ÑÐ»ÑÑÐ¸Ñ
ÑÐ¾Ð·Ð½Ð¸ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð´Ð°Ð¶Ð¸
ÑÐ¾Ð½Ð´Ð¾Ð²ÑÐ¹ ÑÑÐ½Ð¾Ðº Ð¡Ð¨Ð
Ð´ÐµÑÐ¸Ð²Ð°ÑÐ¸Ð²Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¾ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð° Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸ÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ ÐµÐ³Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÑÐ»Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ.
 ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÑÑÑÐ¿Ð°ÑÑ ÐºÑÑÐ¿Ð½ÑÐµ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ðµ Ð¸ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÐµ Ð½ÐµÑÑÑÐ½ÑÐµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, ÑÐ°ÐºÐ¸Ðµ, ÐºÐ°Ðº: ÐÐÐ Â«ÐÐ°Ð·Ð¿ÑÐ¾Ð¼Â», ÐÐÐ Â«ÐÐ Â«Ð Ð¾ÑÐ½ÐµÑÑÑÂ»Â», ÐÐÐ Â«ÐÑÐºÐ¾Ð¹Ð»Â», Sinopec Corp., British Petroleum, Royal Dutch Shell. ÐÑÐ½Ð¾Ð²ÑÐ²Ð°ÑÑÑ Ð½Ð° Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐµ Ð¸ Ð³Ð¾Ð´Ð¾Ð²ÑÑ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð¾ÑÑÐµÑÐ¾Ð² Ð²ÑÑÐµÐ¿ÐµÑÐµÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹ Ð±ÑÐ»Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹, Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð. ÐÑÐ»Ð¸ÐºÐ° Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¾ ÐµÐ³Ð¾ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ Ð½Ð° Ð¾ÑÐµÐ½ÐºÑ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹. ÐÑÐ»Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ Ð¾ÑÐ½Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð¸ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ°.
title: Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº ÑÑÑÐ´Ð¾Ð² Ð¿Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°Ð¼ ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸, Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð½Ð¾Ð¹ 75-Ð»ÐµÑÐ¸Ñ ÑÐ¾ Ð´Ð½Ñ ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð´Ð¾ÐºÑÐ¾ÑÐ° ÑÐµÐ»ÑÑÐºÐ¾Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½Ð°ÑÐº, Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÐ° ÐÐ°ÐºÐ°Ð¹ Ð. Ð.
Creators: name: ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ, Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð½Ð°Ñ 75-Ð»ÐµÑÐ¸Ñ ÑÐ¾ Ð´Ð½Ñ ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð´Ð¾ÐºÑÐ¾ÑÐ° ÑÐµÐ»ÑÑÐºÐ¾Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÑ  Ð½Ð°ÑÐº, Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÐ° ÐÐ°ÐºÐ°Ð¹ Ð. Ð. (2022; ÐÐ¾ÑÐºÐ²Ð°)
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2022
Subjects: ÐÐ°ÐºÐ°Ð¹, ÐÐ½Ð°ÑÐ¾Ð»Ð¸Ð¹ ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸ÑÐ¾Ð²Ð¸Ñ, 1946-2020
Ð¶Ð¸Ð²Ð¾ÑÐ½Ð¾Ð²Ð¾Ð´ÑÑÐ²Ð¾
ÑÐµÐ»ÑÑÐºÐ¾Ðµ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²Ð¾

description: Ð ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÑÐ°ÑÑÐ¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¶Ð¸Ð²Ð¾ÑÐ½Ð¾Ð²Ð¾Ð´ÑÑÐ²Ð°,
Ð¾ÑÐ²ÐµÑÐ°ÑÑÐ¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð·Ð¾Ð¾ÑÐµÑÐ½Ð¸Ð¸, ÑÐ°Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ñ, ÑÐµÐ»ÐµÐºÑÐ¸Ð¸, Ð³ÐµÐ½ÐµÑÐ¸ÐºÐ¸, ÐºÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ Ð¶Ð¸Ð²Ð¾ÑÐ½ÑÑ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°. Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²Ð°.
A photometric study of the southern Blazhko star SS For Unambiguous detection of quintuplet components
Creators: name: Kolenberg, Katrien
name: Guggenberger, Elisabeth
name: Medupe, Thebe
name: Lenz, Patrick
name: Schmitzberger, Lukas
name: Shobbrook, Robert
name: Beck, Paul
name: Ngwato, Boitumelo
name: Lub, Jan
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present our analysis of photometric data in the Johnson B and V filter of the southern Blazhko star SS For. In parallel, we analyzed the V observations obtained with the ASAS-3 photometry of the star gathered between 2000 and 2008. In the frequency spectra resulting from a Fourier analysis of our data, the triplet structure is detectable up to high order, both in the B and V data. Moreover, we find evidence for quintuplet components. We confirm from our data that the modulation components decrease less steeply than the harmonics of the main frequency. We derived the variations of the Fourier parameters quantifying the light curve shape over the Blazhko cycle. There is good agreement between the spectroscopic abundance and the metallicity determined from the Fourier parameters of the average light curve. SS For is peculiar as a Blazhko star because of its strong variations around minimum light.
description: 15 pages, 14 figures, accepted for publication in MNRAS
Triggered Star Formation and Evolution of T-Tauri stars in and around Bright-Rimmed Clouds
Creators: name: Chauhan, Neelam
name: Pandey, A. K.
name: Ogura, K.
name: Ojha, D. K.
name: Bhatt, B. C.
name: Ghosh, S. K.
name: Rawat, P. S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The aim of this paper is to quantitatively testify the "{\it small-scale sequential star formation}" hypothesis in and around bright-rimmed clouds (BRCs). As a continuation of the recent attempt by Ogura et al. (2007, Paper I), we have carried out $BVI_{c}$ photometry of four more BRC aggregates along with deeper re-observations of 2 previously observed BRCs. Again quantitative age gradients are found in almost all the BRCs studied in the present work. Archival Spitzer/IRAC data also support this result. The global distribution of NIR excess stars in each HII region studied here clearly shows evidence that a series of radiation driven implosion (RDI) processes proceeded in the past from near the central O star(s) towards the peripheries of the HII region. We found that in general weak-line T-Tauri stars (WTTSs) are somewhat older than classical T-Tauri stars (CTTSs). Also the fraction of CTTSs among the T-Tauri stars (TTSs) associated with the BRCs is found to decrease with age. These facts are in accordance with the recent conclusion by Bertout et al. (2007) that CTTSs evolve into WTTSs. It seems that in general the EW of H$α$ emission in TTSs associated with the BRCs decreases with age. The mass function (MF) of the aggregates associated with the BRCs of the morphological type "A" seems to follow that found in young open clusters, whereas "B/C" type BRCs show significantly steeper MF.
description: Accepted for publication in MNRAS, 29 pages, 18 figures
title: Ð¡Ð¾Ð±ÑÑÐ¸Ñ Ð² ÐÐ¾Ð½ÐºÐ¾Ð½Ð³Ðµ Ð² 2014 Ð³Ð¾Ð´Ñ Ð² ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ Ð¿ÐµÑÐ¸Ð¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÐµÑÐ°ÑÐ½ÑÑ Ð¸Ð·Ð´Ð°Ð½Ð¸ÑÑ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÑÑÐ°ÑÐ¾Ð²Ð°, Ð¡Ð¾ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐ¸ÑÐ°Ð¹
ÐÐ¾Ð½ÐºÐ¾Ð½Ð³
Â«ÑÐµÐ²Ð¾Ð»ÑÑÐ¸Ñ Ð·Ð¾Ð½ÑÐ¸ÐºÐ¾Ð²Â»
Ð¿ÑÐ¾ÑÐµÑÑÑ
ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ðµ Ð¿ÐµÑÐ°ÑÐ½ÑÐµ Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ

description: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð¾ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ðµ Ð¾ÑÐ²ÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð² ÐÐ¾Ð½ÐºÐ¾Ð½Ð³Ðµ Ð² 2014 Ð³Ð¾Ð´Ñ Ð² ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ Ð³Ð°Ð·ÐµÑÐ°Ñ. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿ÑÐ±Ð»Ð¸ÐºÐ°ÑÐ¸Ð¸ ÑÐµÑÑÑÐµÑ Ð¿Ð¾Ð¿ÑÐ»ÑÑÐ½ÑÑ Ð¿ÐµÑÐ°ÑÐ½ÑÑ Ð¸Ð·Ð´Ð°Ð½Ð¸Ð¹: Â«ÐÑÐ³ÑÐ¼ÐµÐ½ÑÑ Ð¸ Ð¤Ð°ÐºÑÑÂ», Â«ÐÐ¾Ð²Ð°Ñ Ð³Ð°Ð·ÐµÑÐ°Â», Â«ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð´Ð½ÐµÐ²Ð½Ð¸ÐºÂ», Â«ÐÐ¾Ð¼Ð¼ÐµÑÑÐ°Ð½ÑÂ». ÐÐ¾ Ð¸ÑÐ¾Ð³Ð°Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð¾Ð¶Ð½Ð¾ ÑÐ´ÐµÐ»Ð°ÑÑ Ð²ÑÐ²Ð¾Ð´, ÑÑÐ¾ ÑÐ°Ð·Ð½Ð¸ÑÐ° Ð¿ÑÐ±Ð»Ð¸ÐºÐ°ÑÐ¸Ð¹ Ð² ÑÐ¾Ð¼, ÐºÐ°Ðº Ð¸Ð¼ÐµÐ½Ð½Ð¾ Ð°Ð²ÑÐ¾ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð³Ð°Ð·ÐµÑ ÑÐ°ÑÑÑÐ°Ð²Ð»ÑÑÑ Ð°ÐºÑÐµÐ½ÑÑ Ð¸ ÐºÐ°ÐºÐ¾Ð³Ð¾ ÑÐ¾Ð´Ð° Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð²ÑÐ²Ð¾Ð´ÑÑ Ð½Ð° Ð¿ÐµÑÐ²ÑÐ¹ Ð¿Ð»Ð°Ð½.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ²ÐµÑÑ ÑÐ¸ÑÐ¾ÐºÐ¾Ð¿Ð¾Ð»Ð¾ÑÐ½ÑÑ Ð°Ð½ÑÐµÐ½Ð½ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ»ÐµÐºÑÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¾ Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐµÐ»ÑÑÐºÐ°Ñ, Ð®Ð»Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐ½ÑÐµÐ½Ð½Ñ ÑÐ¸ÑÐ¾ÐºÐ¾Ð¿Ð¾Ð»Ð¾ÑÐ½ÑÐµ
Ð­Ð»ÐµÐºÑÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ° Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ
ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¾ Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ²ÐµÑÑÑÐ¸ÑÐ¾ÐºÐ¾Ð¿Ð¾Ð»Ð¾ÑÐ½ÑÑ Ð°Ð½ÑÐµÐ½Ð½ Ð´Ð²ÑÑ ÑÐ¸Ð¿Ð¾Ð² Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿Ð°ÐºÐµÑÐ° CST Microwave Studio, Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ Ð²ÑÐ¾Ð´Ð½ÑÐµ Ð¸ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½ÑÐµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ñ ÑÐ°ÑÑÐµÑÐ½ÑÐ¼Ð¸, Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð°Ð½ÑÐµÐ½Ð½Ñ Ð½Ð° ÐµÐµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´Ñ Ð¾Ð´Ð° Ðº ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð·Ð°ÑÐ¾Ð²Ð°, Ð­Ð»ÑÐ¼Ð¸ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ°
Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿Ð¾Ð´Ñ Ð¾Ð´
ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ðµ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ°
Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ
Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ°

description: ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â«ÐÑÐ»ÐºÐ¾Ð²ÑÐºÐ¾Ðµ ÑÐ¾ÑÑÐµ 19Â». Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ðº ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â«ÐÑÐ»ÐºÐ¾Ð²ÑÐºÐ¾Ðµ ÑÐ¾ÑÑÐµ 19Â». Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð·Ð°ÑÑÐ°ÑÑ Ð½Ð° Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ðº ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â«ÐÑÐ»ÐºÐ¾Ð²ÑÐºÐ¾Ðµ ÑÐ¾ÑÑÐµ 19Â». Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ðº ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ° Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°ÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â«ÐÑÐ»ÐºÐ¾Ð²ÑÐºÐ¾Ðµ ÑÐ¾ÑÑÐµ 19Â».
title: ÐÑÐ°ÑÐ¸ÐºÐ° Ð² Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐµ Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð¤ÐµÐ´Ð¾ÑÐ¾Ð²Ð°, ÐÐ°Ð»ÐµÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ°ÑÐ¸Ð½Ð½Ð°Ñ Ð³ÑÐ°ÑÐ¸ÐºÐ°
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
ÐÐ½ÑÐµÑÑÐµÐ¹ÑÑ
Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ðµ Ð¸Ð³ÑÑ
ÐºÐ¾Ð³Ð½Ð¸ÑÐ¸Ð²Ð½ÑÐ¹ Ð¿Ð¾Ð´Ñ Ð¾Ð´

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÑÐ¸Ð¿Ð° Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ¾Ð² Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ Ð¸Ð³ÑÐ¾Ð²ÑÑ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð½Ð° ÐºÐ¾Ð³Ð½Ð¸ÑÐ¸Ð²Ð½ÑÐµ ÑÑÐ½ÐºÑÐ¸Ð¸ ÑÑÐ°ÑÐ¸ÑÑÑ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¸Ð³ÑÑ, Ð¾Ð±ÑÑÐ°ÑÑÐµÐ¹ Ð¾ÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿ÐµÑÐ²Ð¾Ð¹ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸ÑÑ.Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ ÑÐ¸Ð¿Ð° Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ¾Ð² ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ (Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ) Ð½Ð° Ð¿ÑÐ¾ÑÐµÑÑÑ Ð·Ð°Ð¿Ð¾Ð¼Ð¸Ð½Ð°Ð½Ð¸Ñ Ð¸ Ð²Ð¾ÑÐ¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ¸Ð¿Ð¾Ð² Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ¾Ð².
title: ÐÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð²Ð½Ð¾-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ½ÑÐ¹ Ð¿Ð¾Ð´Ñ Ð¾Ð´ Ð² Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð½Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÑÐ¾ÑÐ¾Ð½Ðµ ÑÐµÑÐ¸ Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ ÑÑÐ°Ð½ÑÑÐ·ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ° ÐºÐ°Ðº Ð²ÑÐ¾ÑÐ¾Ð³Ð¾ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð³Ð¾ Ð² Ð²ÑÐ·Ðµ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ
title: Communicative and active approach in teaching of pronunciation side of speech when learning french as a second foreign language at the university of physical education
Creators: name: ÐÐµÐ»ÑÐºÐ¾Ð²Ð°, Ð.
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: Ð²ÑÐ¾ÑÐ¾Ð¹ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¹ ÑÐ·ÑÐº
ÑÐ¾Ð½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð½Ð°Ð²ÑÐº
Ð¸Ð½ÑÐµÑÑÐµÑÐµÐ½ÑÐ¸Ñ

description: Ð ÑÑÐ°ÑÑÐµ Ð¿Ð¾Ð´ÑÐµÑÐºÐ¸Ð²Ð°ÐµÑÑÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð¾Ð²Ð»Ð°Ð´ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð½Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÑÐ¾ÑÐ¾Ð½Ð¾Ð¹ ÑÐµÑÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸, Ð½Ð°ÑÐ¸Ð½Ð°ÑÑÐ¸Ð¼Ð¸ Ð¸Ð·ÑÑÐ°ÑÑ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¹ ÑÐ·ÑÐº Ð² Ð²ÑÐ·Ðµ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ.
description: The article emphasizes the need to master the pronunciation side of speech by students beginning to study a second foreign language at the University of physical education.
The dynamics of quark-gluon plasma and AdS/CFT
Creators: name: Janik, Romuald A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: In these pedagogical lectures, we present the techniques of the AdS/CFT correspondence which can be applied to the study of real time dynamics of a strongly coupled plasma system. These methods are based on solving gravitational Einstein's equations on the string/gravity side of the AdS/CFT correspondence. We illustrate these techniques with applications to the boost-invariant expansion of a plasma system. We emphasize the common underlying AdS/CFT description both in the large proper time regime where hydrodynamic dynamics dominates, and in the small proper time regime where the dynamics is far from equilibrium. These AdS/CFT methods provide a fascinating arena interrelating General Relativity phenomenae with strongly coupled gauge theory physics.
description: 35 pages, 3 figures. Lectures at the 5th Aegean summer school, `From gravity to thermal gauge theories: the AdS/CFT correspondence'. To appear in the proceedings in `Lecture Notes in Physics'
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼Ð¾Ð´ÑÐ»Ñ Â«Ð¾Ð¿ÑÐ¾Ñ ÑÐ´Ð°Ð»ÑÐ½Ð½ÑÑ ÑÐµÐ¿Ð»Ð¾Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÐµÐ¹Â»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÐµÐ±ÑÐ¾Ð², ÐÐ»ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ
ÑÑÐµÑÐ° ÐÐÐ¥
Ð¿ÑÐ¾ÑÐ¾ÐºÐ¾Ð»Ñ
Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð²Ð¾Ð¿ÑÐ¾Ñ Ð¾ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð² ÑÑÐµÑÐµ Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²Ð° (ÐÐÐ¥). ÐÐ° ÑÐµÐ³Ð¾Ð´Ð½ÑÑÐ½Ð¸Ð¹ Ð´ÐµÐ½Ñ Ð±Ð¾Ð»ÑÑÐ¸Ð½ÑÑÐ²Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² ÐÐÐ¥ Ð´ÐµÐ»Ð°ÐµÑÑÑ Ð²ÑÑÑÐ½ÑÑ. ÐÐ´Ð½Ð°ÐºÐ¾, ÑÐµÐºÑÑÐ¸Ð¹ ÑÑÐ¾Ð²ÐµÐ½Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð¼Ð½Ð¾Ð³Ð¸Ðµ Ð¸Ð· Ð½Ð¸Ñ: ÑÐ°ÑÑÐµÑ Ð¸ Ð½Ð°ÑÐ¸ÑÐ»ÐµÐ½Ð¸Ðµ Ð¿Ð»Ð°ÑÐµÐ¶ÐµÐ¹ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸ÐµÐ¼, Ð´Ð¸ÑÐ¿ÐµÑÑÐµÑÑÐºÐ°Ñ ÑÐ»ÑÐ¶Ð±Ð°, ÑÐ±Ð¾Ñ Ð¸ ÑÐ°Ð±Ð¾ÑÐ° Ñ Ð´Ð°Ð½Ð½ÑÐ¼Ð¸ ÑÑÐµÑÑÐ¸ÐºÐ¾Ð² Ð²Ð¾Ð´Ñ, ÑÐµÐ¿Ð»Ð° Ð¸ Ð³Ð°Ð·Ð°, ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð¸Ð·Ð²ÐµÑÐµÐ½Ð¸Ð¹ Ð´Ð»Ñ Ð¶Ð¸Ð»ÑÑÐ¾Ð².
title: ÐÐµÑÐ¾Ð´Ñ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ñ ÑÐµÑÐµÐ²ÑÑ Ð°ÑÐ°Ðº. Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð² ÐºÐ¸Ð±ÐµÑÐ±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð£ÐÐ¡Ð 10.00.00 Â«ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑÂ» Ð¿Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°Ð¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð², Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð², ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð²
titleType: Subtitle
Creators: name: ÐÐ»Ð°ÑÐ¾Ð½Ð¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ
ÐÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑ

description: Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÑÑ Ð² Ð½Ð°ÑÑÐ¾ÑÑÐµÐµ Ð²ÑÐµÐ¼Ñ. ÐÐ°ÑÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸. Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Â«ÐÐµÑÐ¾Ð´Ñ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ñ ÑÐµÑÐµÐ²ÑÑ Ð°ÑÐ°Ðº. Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð² ÐºÐ¸Ð±ÐµÑÐ±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸Â» Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐ¼ Ð¼ÐµÑÐ¾Ð´Ð°Ð¼ Ð¸ ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÑÐµÐ´ÑÑÐ² Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ.
Rotationally Warm Molecular Hydrogen in the Orion Bar
Creators: name: Shaw, Gargi
name: Ferland, G. J.
name: Henney, W. J.
name: Stancil, P. C.
name: Abel, N. P.
name: Pellegrini, E. W.
name: Baldwin, J. A.
name: van Hoof, P. A. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Orion Bar is one of the nearest and best-studied photodissociation or photon-dominated regions (PDRs). Observations reveal the presence of H2 lines from vibrationally or rotationally excited upper levels that suggest warm gas temperatures (400 to 700 K). However, standard models of PDRs are unable to reproduce such warm rotational temperatures. In this paper we attempt to explain these observations with new comprehensive models which extend from the H+ region through the Bar and include the magnetic field in the equation of state. We adopt the model parameters from our previous paper which successfully reproduced a wide variety of spectral observations across the Bar. In this model the local cosmic-ray density is enhanced above the galactic background, as is the magnetic field, and which increases the cosmic-ray heating elevating the temperature in the molecular region. The pressure is further enhanced above the gas pressure in the H+ region by the momentum transferred from the absorbed starlight. Here we investigate whether the observed H2 lines can be reproduced with standard assumptions concerning the grain photoelectric emission. We also explore the effects due to the inclusion of recently computed H2 + H2, H2 + H and H2 + He collisional rate coefficients.
description: Accepted for publication in ApJ (34 pages, including 16 figures)
Machine learning in transcriptome analysis using long RNA sequencing data
Creators: name: Hafezqorani, Saber
Publisher: name: University of British Columbia
Year: 2024

description: The advent of long-read RNA sequencing technologies has advanced transcriptomic research by enabling the sequencing of entire transcripts. This advancement holds the promise of uncovering novel insights into the complex nature of eukaryotic transcriptomes, characterized by phenomena such as alternative splicing and intron retention. However, the vast amounts of data generated by these technologies necessitates the development of sophisticated tools for effective data analysis. This thesis addresses these challenges through two main objectives: the development of a novel simulator for long-read RNA sequencing data, capable of accurately mimicking transcriptome-specific features and the application of deep learning techniques for the robust analysis of RNA sequencing data. The first objective addresses the need for a simulator tailored specifically for RNA sequencing data from Oxford Nanopore Technologies, aiming to create a tool that not only generates reads mimicking real sequencing outputs, but also incorporates critical transcriptomic features such as expression levels and intron retention events. This simulator serves as a resource for the development and refinement of transcriptome analysis tools, offering a cost-effective alternative to extensive sequencing experiments to generate ground-truth data for benchmarking. The second objective explores the potential of deep learning in transcriptomics, focusing on the development of a nucleotide sequence embedding method. It aims to capture the complex, long-term dependencies within sequences, a task that has proven challenging due to the variable length and intricate nature of RNA sequences. By leveraging deep learning's capacity to learn feature representations implicitly, this research seeks to enhance the accuracy and efficiency of sequence classification and clustering tasks within transcriptomic studies.
Multi-Stream Inflation
Creators: name: Li, Miao
name: Wang, Yi
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We propose a "multi-stream" inflation model, which is a double field model with spontaneous breaking and restoration of an approximate symmetry. We calculate the density perturbation and non-Gaussianity in this model. We find that this model can have large, scale dependent, and probably oscillating non-Gaussianity. We also note that our model can produce features in the CMB power spectrum and hemispherical power asymmetry.
description: 14 pages, 2 figures; v2: references added; v3: final version to appear on JCAP
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð¿Ð»Ð°Ð½Ð° ÐµÑ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¤Ð¾Ð¼Ð¸Ð½ÑÑ, ÐÐ»ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ
ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ
ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ°
development strategy
strategy
development

description: Ð Ð°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð² ÑÐµÐ±Ðµ Ð¾ÑÐ½Ð¾Ð²Ð¾Ð¿Ð¾Ð»Ð°Ð³Ð°ÑÑÐ¸Ðµ Ð¿Ð¾Ð½ÑÑÐ¸Ñ, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·ÑÑÑÐ¸Ðµ ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐ¸Ð¹ Ð¿Ð»Ð°Ð½ ÐµÐµ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð¢Ð°ÐºÐ¶Ðµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð°Ñ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¹ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«Ð Ð¾ÑÑÐµÐ»ÐµÐºÐ¾Ð¼Â» Ð½Ð° Ð¿ÑÐµÐ´Ð¼ÐµÑ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ, Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ Ð´Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÐµÐµ Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ð¸.
description: The work contains the basic concepts that characterize the company's development strategy and further plan its implementation. Also includes detailed classification of existing development strategies, defined the concept of the strategic plan of the enterprise. The analysis of the company PJSC "Rostelecom" to assess the effectiveness of the current development strategy highlights the main issues and recommendations for its modernization.
Transformation from spots to waves in a model of actin pattern formation
Creators: name: Whitelam, Stephen
name: Bretschneider, Till
name: Burroughs, Nigel J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Subcellular Processes (q-bio.SC)
subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Biological sciences
subject: FOS: Physical sciences

description: Actin networks in certain single-celled organisms exhibit a complex pattern-forming dynamics that starts with the appearance of static spots of actin on the cell cortex. Spots soon become mobile, executing persistent random walks, and eventually give rise to traveling waves of actin. Here we describe a possible physical mechanism for this distinctive set of dynamic transformations, by equipping an excitable reaction-diffusion model with a field describing the spatial orientation of its chief constituent (which we consider to be actin). The interplay of anisotropic actin growth and spatial inhibition drives a transformation at fixed parameter values from static spots to moving spots to waves.
Additional file 2 of Myeloid CCN3 protects against aortic valve calcification
Creators: name: Tu, Peinan
name: Xu, Qian
name: Zhou, Xianming
name: Villa-Roel, Nicolas
name: Kumar, Sandeep
name: Dong, Nianguo
name: Jo, Hanjoong
name: Ou, Caiwen
name: Lin, Zhiyong
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology

description: Additional file 1. Fig. S1: Murine CAVD model. A. Study protocol for CAVD in mice. B. Representative images of aortic valvular regurgitation detected by Spectral Doppler in mice. An entire peak of regurgitation was defined as severe regurgitation (upper panel), and a partial peak was defined as mild regurgitation (lower panel). C. Distribution of aortic valve regurgitation in control and Mye-CCN3-KO mice (n=16, 8 males and 8 females). Control: LysmCre/Cre mice; Mye-CCN3-KO: Myeloid specific CCN3 knock out mice. Fig. S2: Plasma lipid profile of mice post 40 weeks of high fat diet feeding. All Statistical analysis were two-way ANOVA followed by Sidak multiple comparison test. N=biological replicates. CHOL indicates cholesterol; TG, Triglyceride; HDLC: High density lipoprotein cholesterol; none HDLc: Non-high-density lipoprotein cholesterol; LDLc, Low-Density Lipoprotein Cholesterol; Control: LysmCre/Cre mice; Mye-CCN3-KO: Myeloid specific CCN3 knock out mice. Fig. S3: Loss of CCN3 causes an increase of macrophages migration in vivo and vitro. A. Representative immunostaining for CD68 on aortic valve of Control and Mye-CCN3-KO mice. Scale bar=100μm. Quantification of the relative fold change of positive stained area to the entire valve leaflet area in comprision to the control group (n=5). B. Scratch assay for primary macrophages cultured in DMEM. Images were analyzed with ImageJ. Scale bar: 200μm; n=6. Data analysis were unpaired Student’s t-test. N=biological replicates. Control: LysmCre/Cre mice; Mye-CCN3-KO: Myeloid specific CCN3 knock out mice; Mφlysm: BMDMs from Control mice; Mφ△CCN3: BMDMs from Mye-CCN3-KO mice. *p<0.05. **p<0.01. Fig. S4: Characterization of bone marrow-derived macrophages. A. Characterization of primary murine macrophages by flow cytometry. Percentage of MHC II+ and CD206+ within CD11b+ and F4/80+ controls (n=5). B. Relative CCN3, F4/80, IL-10 and TNFα expression in BMDMs (n=6). All data analyses were unpaired Student’s t-test. N=biological replicates. Mφlysm: BMDMs from Control mice; Mφ△CCN3: BMDMs from Mye-CCN3-KO mice. ****p<0.0001. Fig. S5: Verification of the blocking efficacy of BMP2 nAb in vitro. A. Diagram for verification of BMP2 nAb in vitro. B. BMDMs were transfected with pGL3 luciferase plasmid. After 24 hours, cells were treated with BMP2 (10 ng/ml) in the presence or absence of BMP2 nAb (1μg/ml) for 24 hours prior to measuring luciferase activity (n=4). *p<0.05.