cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
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¸ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° Ð¸ÑÐ¿Ð°Ð½ÑÐºÐ¾Ð¹ ÐºÑÑ Ð½Ð¸ Ð½Ð° 65 Ð¼ÐµÑÑ Ð² Ð³. Ð¡Ð¾ÑÐ½Ð¾Ð²ÑÐ¹ ÐÐ¾Ñ ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¾Ð½Ð¸Ð½Ð°, 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: 2016
Subjects: ÑÐµÑÑÐ¾ÑÐ°Ð½
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description: Ð Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ 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 ÑÐµÑÑÐ¾ÑÐ°Ð½Ð°, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð¿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. 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, ÐµÐ³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸.
Marte, tracce organiche in fumo
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

Identificato un minerale che, quando riscaldato, distrugge i composti organici. La scoperta, pubblicata su Astrobiology, potrebbe avere conseguenze per il rover Curiosity della NASA e per le future missioni, come ExoMars, dedicate alla ricerca di tracce di vita sul Pianeta rosso
MAVEN completa la prima immersione
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2015

MAVEN, la missione NASA che indaga l’atmosfera marziana per capire quale sia stata la sua evoluzione e quale sia il suo attuale stato, ha completato la prima campagna di raccolta dati, effettuata attraversando l’atmosfera del pianeta rosso, fino a spingersi ad una distanza di soli 125 chilometri dalla sua superficie
Più vicini alla stella Beta Pictoris
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Un gruppo di ricercatori dell'Università dell'Ariziona ha usato il telescopio orbitante di NASA ed ESA per scattare una foto ancora più dettagliata in luce visibile del grande disco di gas e polvere che circonda la giovanissima stella
Un nuovo aspetto per l’eliosfera
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Una nuova ricerca suggerisce che il campo magnetico solare influisca sulla forma a larga scala dell'eliosfera. Nel nuovo modello il campo magnetico comprime il vento solare lungo gli assi nord e sud, producendo due getti che vengono poi spinti verso il basso dal flusso del mezzo interstellare attraverso cui si muove l'eliosfera
Tidal disruption of globular clusters in dwarf galaxies with triaxial dark matter haloes
Creators: name: Penarrubia, Jorge
name: Walker, Matthew G.
name: Gilmore, Gerard
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We use N-body simulations to study the tidal evolution of globular clusters (GCs) in dwarf spheroidal (dSph) galaxies. Our models adopt a cosmologically motivated scenario in which the dSph is approximated by a static NFW halo with a triaxial shape. We apply our models to five GCs spanning three orders of magnitude in stellar density and two in mass, chosen to represent the properties exhibited by the five GCs of the Fornax dSph. We show that only the object representing Fornax's least dense GC (F1) can be fully disrupted by Fornax's internal tidal field--the four denser clusters survive even if their orbits decay to the centre of Fornax. For a large set of orbits and projection angles we examine the spatial and velocity distribution of stellar debris deposited during the complete disruption of an F1-like GC. Our simulations show that such debris appears as shells, isolated clumps and elongated over-densities at low surface brightness (>26 mag/arcsec^2), reminiscent of substructure observed in several MW dSphs. Such features arise from the triaxiality of the galaxy potential and do not dissolve in time. The kinematics of the debris depends strongly on the progenitor's orbit. Debris associated with box and resonant orbits does not display stream motions and may appear "colder"/"hotter" than the dSph's field population if the viewing angle is perpendicular/parallel to progenitor's orbital plane. In contrast, debris associated with loop orbits shows a rotational velocity that may be detectable out to few kpc from the galaxy centre. Chemical tagging that can distinguish GC debris from field stars may reveal whether the merger of GCs contributed to the formation of multiple stellar components observed in dSphs.
description: accepted by MNRAS, 22 pages
A volunteer programme for patients in a provincial mental hospital : a review of organization and services contributed, based on some current developments at Essondale, B.C., 1954-58
Creators: name: Ross, Robert MacGregor
Publisher: name: University of British Columbia
Year: 2012

description: The goal of hospital treatment is the return of its patients to their community in a healthy, happy condition. This can be a particularly difficult objective to achieve in the case of mental illness because of traditional hospital isolation, and fear and misconceptions about on the part of the public. More and more it is being realized that if there is to be effective rehabilitation of the mentally ill, there must be greater understanding and acceptance of mental illness by their communities. This study examines the recently-developed volunteer programme at the Provincial Mental Hospital, (Essondale, B.C.,) sponsored by the Canadian Mental Health Association. It describes the programme's organization, and its activities aimed at bringing the community to the patient, as well as interpreting hospital and patient needs to the community. The method used in the study began with a review of professional and other literature in order to learn what volunteer services were being offered in mental hospital settings elsewhere. A questionnaire was then completed and interviews with key people in the volunteer movement conducted, in order to compile details of its development, organization and acceptance by hospital management and staff as a "treatment extra". In order to illustrate volunteer activities and potentials in detail, the focus was then narrowed to the study of one particular ward (Chapter 3.) Types of patients were described experimentally as belonging to behavior groups observed on the ward, such as "attention seekers" and "rescue seekers." (The possibility of a ward classification according to the various categories of mental illness such as chronic brain syndromes, psychotic disorders, etc., was considered but discarded because the required information was not available.) Ways in which volunteers can help the patients in the various behavior groups when visiting and assisting in occupational therapy are discussed, using two case examples for illustration. The study confirmed the general thinking that the volunteer programme is contributing a very useful service to the hospital treatment programme. In the concluding chapter some suggestions are offered towards increasing the effectiveness of this growing volunteer service. These are related to a problem common to all volunteer work, namely, sustaining the interest of volunteers. In addition, suggestions are made as to some ways in which the volunteers could work with the Social Service Department in this hospital setting.
Il super vento che spazza la galassia
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Il team internazionale di astronomi guidato da Emanuele Nardini e a cui hanno partecipato ricercatori italiani e dell'INAF, ha studiato le proprietà del poderoso vento emesso dal buco nero supermassivo al centro di una galassia misurandone, per la prima volta,  l’intensità e rivelando anche come si propaghi dal buco nero in tutte le direzioni. Il lavoro è pubblicato nell'ultimo numero della rivista Science
title: Performance Characterization of Complex Fuel Port Geometries for Hybrid Rocket Fuel Grains
Creators: name: Bath, Andrew
Publisher: name: Utah State University
Year: 2012

description: This research investigated the 3D printing and burning of fuel grains with complex geometry and the development of software capable of modeling and predicting the regression of a cross-section of these complex fuel grains. The software developed did predict the geometry to a fair degree of accuracy, especially when enhanced corner rounding was turned on. The model does have some drawbacks, notably being relatively slow, and does not perfectly predict the regression. If corner rounding is turned off, however, the model does become much faster; although less accurate, this method does still predict a relatively accurate resulting burn geometry, and is fast enough to be used for performance-tuning or genetic algorithms. In addition to the modeling method, preliminary investigations into the burning behavior of fuel grains with a helical flow path were performed. The helix fuel grains have a regression rate of nearly 3 times that of any other fuel grain geometry, primarily due to the enhancement of the friction coefficient between the flow and flow path.
Tri-Bimaximal Lepton Mixing and Leptogenesis
Creators: name: Sierra, D. Aristizabal
name: Bazzocchi, F.
name: Varzielas, I. de Medeiros
name: Merlo, L.
name: Morisi, S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In models with flavour symmetries added to the gauge group of the Standard Model the CP-violating asymmetry necessary for leptogenesis may be related with low-energy parameters. A particular case of interest is when the flavour symmetry produces exact Tri-Bimaximal lepton mixing leading to a vanishing CP-violating asymmetry. In this paper we present a model-independent discussion that confirms this always occurs for unflavoured leptogenesis in type I see-saw scenarios, noting however that Tri-Bimaximal mixing does not imply a vanishing asymmetry in general scenarios where there is interplay between type I and other see-saws. We also consider a specific model where the exact Tri-Bimaximal mixing is lifted by corrections that can be parametrised by a small number of degrees of freedom and analyse in detail the existing link between low and high-energy parameters - focusing on how the deviations from Tri-Bimaximal are connected to the parameters governing leptogenesis.
description: 29 pages, 6 figures; version 2: references added, minor corrections
Impulso magnetoacustico colto sul fatto
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

Osservati per la prima volta dall’inizio alla fine, grazie alle sonde gemelle Van Allen Probes della NASA, gli effetti sulla magnetosfera terrestre di un’onda d’urto supersonica di vento solare. Grazie a fenomeni di risonanza, riesce ad accelerare gli elettroni a velocità ultrarelativistiche
Analisi chimica della polvere di un pianeta
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Scoperto nel 2012, questo piccole pianeta (un decimo delle dimensioni della Terra) è talmente vicino alla sua calda stella che si sta lentamente sbriciolando e sciogliendo. Nuove osservazioni sveleranno la composizione chimica dei detriti provenienti dalla superficie del pianeta così da avere qualche indizio anche sulla formazione del nostro pianeta
Additional file 1: of C9orf72 deficiency promotes motor deficits of a C9ALS/FTD mouse model in a dose-dependent manner
Creators: name: Shao, Qiang
name: Liang, Chen
name: Chang, Qing
name: Zhang, Wei
name: Yang, Mei
name: Chen, Jian-Fu
Publisher: name: figshare
Year: 2019
Subjects: subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Science Policy
subject: Mental Health

description: Figure S1. Characterization of C9-BAC mice with C9orf72 dose reduction. (A) Quantification of C9orf72/Atg101 protein levels. Data are presented as mean ± SEM from three independent experiments. (B, C) Body weight of female (B) and male (C) mice at 4 months of age. (D-G) Open field test was performed on 4-month-old mice to examine the total distance traveled (E), distance traveled in the center (F), and percentage of time spent in the center (G). (H, I) Quantification of the maximal g force from five trials of rotarod assay. C9orf72 deficiency decreases the maximal g force of C9-BAC female mice in a dose-dependent manner. All data are presented as mean ± SEM using numbers (n) of mice as indicated. Statistical analyses were performed with one-way ANOVA with Bonferroni’s post hoc test (*p < 0.05, **p < 0.01, ***p < 0.001, n.s represents no significant difference detected). (PDF 2855 kb)
Temperature dependence of antiferromagnetic susceptibility in ferritin
Creators: name: Silva, N. J. O.
name: Millan, A.
name: Palacio, F.
name: Kampert, E.
name: Zeitler, U.
name: Rakoto, H.
name: Amaral, V. S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We show that antiferromagnetic susceptibility in ferritin increases with temperature between 4.2 K and 180 K (i. e. below the Néel temperature) when taken as the derivative of the magnetization at high fields ($30\times10^4$ Oe). This behavior contrasts with the decrease in temperature previously found, where the susceptibility was determined at lower fields ($5\times10^4$ Oe). At high fields (up to $50 \times10^4$ Oe) the temperature dependence of the antiferromagnetic susceptibility in ferritin nanoparticles approaches the normal behavior of bulk antiferromagnets and nanoparticles considering superantiferromagnetism, this latter leading to a better agreement at high field and low temperature. The contrast with the previous results is due to the insufficient field range used ($< 5 \times10^4$ Oe), not enough to saturate the ferritin uncompensated moment.
description: 7 pages, 7 figures, accepted in Phys. Rev. B
title: ÐÐ±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¾Ð±Ð»ÐµÐ³ÑÐµÐ½Ð½ÑÑ Ð¼Ð½Ð¾Ð³Ð¾Ð¿ÑÑÑÐ¾ÑÐ½ÑÑ Ð¿Ð»Ð¸Ñ Ð¿ÐµÑÐµÐºÑÑÑÐ¸Ð¹
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð ÑÐ¶Ð¾Ð² , ÐÐ»ÐµÐºÑÐ°Ð½Ð´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ÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ½ÑÐµ
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description: Ð Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ½ÑÑ Ð¼Ð½Ð¾Ð³Ð¾Ð¿ÑÑÑÐ¾ÑÐ½ÑÑ Ð¿Ð»Ð¸Ñ Ð¿ÐµÑÐµÐºÑÑÑÐ¸Ð¹. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ Ð¾Ð±Ð»ÐµÐ³ÑÐµÐ½Ð½ÑÑ Ð¸Ð·Ð³Ð¸Ð±Ð°ÐµÐ¼ÑÑ Ð¶ÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð±Ð»ÐµÐ³ÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÐºÑÑÑÐ¸Ñ Ð¸ ÐµÐ³Ð¾ ÑÐ°ÑÑÐµÑÐ° Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ ÐºÐ¾Ð½ÐµÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð². ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð¹ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÐ°ÑÑÐµÑÐ° Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐ¼Ð¸ Ð´Ð°Ð½Ð½ÑÐ¼Ð¸. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ.
Estinzioni di massa dovute alla materia oscura?
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Una ricerca del professor Michael Rampino, biologo dell'Università di New York e del Goddard Institute della NASA, sembra mostrare che i passaggi della Terra attraverso il piano galattico, eventi non molto frequenti, ma prevedibili, possono avere una correlazione diretta e significativa con fenomeni geologici e biologici che avvengono sulla Terra
title: Mechanisms and Signal Transduction Pathways Involved in Bovine Oocyte Activation
Creators: name: Bayles, Ammon Hanson
Publisher: name: Utah State University
Year: 2012

description: In addition to contributing genes at fertilization, the sperm cell induces the oocyte to leave its arrested state and resume metabolism in the process of activation. A hallmark of oocyte activation is a release of intracellular calcium (Ca2+i) from the endoplasmic reticulum. The mediators of oocyte activation have been studied in many animal models, while little is known in the bovine model. Both Src Family Kinase (SFK) and Phospholipase C (PLC) enzymes have been reported to be involved in oocyte activation in other animal models. In this dissertation are described experiments that define the role of SFK and PLC enzymes in the pathway leading to Ca2+i and calcium induced calcium release in bovine oocyte activation. Western blotting was used to discover that SFKs Src, Hck, and Lck are present in matured bovine oocytes, and Src, Blk, and Yes are present in acrosome reacted bovine spermatozoa. The PLC δ1 and δ3 are present in both matured bovine oocytes and spermatozoa. PLC δ4, γ2, and η2 are present in matured bovine oocytes. Microinjecting a known general SFK inhibitor, PP2, significantly decreases both Ca2+i and cleavage rates. Microinjecting a 13 amino acid peptide that mimics the phosphorylated carboxyl terminal region of pp60c-src decreases both Ca2+i and cleavage rates. Microinjecting a downstream substrate of pp60c-src sequestered any signal produced by Src and decreased Ca2+i and cleavage rates. Microinjecting primary antibodies raised against PLC isotypes blocked both Ca2+i and cleavage rates, giving insight to the mechanism of calcium induced calcium release in the bovine model. The PLC isotypes δ3, δ4, and γ2 decreased Ca2+i oscillations and cleavage rates, indicating they are involved in both IP3R and RyR activation. PLC δ4 and η2 did not impact Ca2+i but did significantly decrease cleavage rates. The data presented in this dissertation increase the understanding of the pathway leading to bovine oocyte activation and further confirm that the detailed pathway differs among animal models.
On Domains of PT Symmetric Operators Related to -y''(x) + (-1)^n x^{2n}y(x)
Creators: name: Azizov, Tomas Ya.
name: Trunk, Carsten
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In the recent years a generalization of Hermiticity was investigated using a complex deformation H=p^2 +x^2(ix)^εof the harmonic oscillator Hamiltonian, where εis a real parameter. These complex Hamiltonians, possessing PT symmetry (the product of parity and time reversal), can have real spectrum. We will consider the most simple case: εeven. In this paper we describe all self-adjoint (Hermitian) and at the same time PT symmetric operators associated to H=p^2 +x^2(ix)^ε. Surprisingly it turns out that there are a large class of self-adjoint operators associated to H=p^2 +x^2(ix)^εwhich are not PT symmetric.
title: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²ÐµÐ½Ð½Ð¾ Ð»Ð¾ÐºÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼
title: Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¢Ð¾Ð¼ÑÐ¸Ð½ÑÐºÐ°Ñ, ÐÑÐ¸Ð½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2018
Subjects: Ð¼ÐµÐ·Ð¾ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°
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description: Ð¡Ð¾Ð·Ð´Ð°Ð½Ð¸Ðµ ÑÐ»Ð°Ð±Ð¾ ÑÑÑÑÐºÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¾Ð±ÑÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ (ÑÐ¾ÑÐ·Ð¾Ð²) Ð²Ð¾ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ¹ ÑÑÐµÐ´Ðµ Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ Ð²ÑÑÐ²Ð¸ÑÑ Ð¸ ÑÐ°Ð·ÑÐµÑÐ¸ÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ, Ð½Ð°Ð¿ÑÐ°Ð²Ð¸ÑÑ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÑ. ÐÐ»Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ°ÐºÐ¸Ñ Ð¾Ð±ÑÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÑ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ, Ð°Ð´ÑÐµÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¹ ÑÑÐ±ÑÐµÐºÑÐ°Ð¼ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸, ÑÐ¿Ð¾ÑÐ¾Ð±Ð½ÑÑ ÑÑÐ°ÑÑ Ð¿Ð»Ð°ÑÐ´Ð°ÑÐ¼Ð°Ð¼Ð¸ Ð½Ð¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ°. Ð Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ ÑÐ°ÑÐºÑÑÑÐ¾ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²ÐµÐ½Ð½Ð¾ Ð»Ð¾ÐºÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼: ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð° Ð¸Ñ Ð¿ÑÐ¸Ð½Ð°Ð´Ð»ÐµÐ¶Ð½Ð¾ÑÑÑ Ðº ÑÐ°Ð·Ð²ÐµÑÐ½ÑÑÑÐ¼ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÐ¼ ÑÑÐ±ÑÐµÐºÑÐ°Ð¼, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ð¼ Ð¿Ð¾Ð´ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸ÐµÐ¼ ÑÑÐºÐ¾ÑÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐ¸Ð½Ð´ÑÑÑÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ð¹ (Ð¿Ð»Ð°ÑÐ´Ð°ÑÐ¼Ð°Ð¼ Ð´Ð°Ð½Ð½ÑÑ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð²Ð¾ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ¹ ÑÑÐµÐ´Ðµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸). ÐÐ°Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ²Ð»ÑÑÑÑÑ ÐºÐ»ÑÑÐµÐ²ÑÐ¼ ÑÑÑÑÐºÑÑÑÐ½ÑÐ¼ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð¼ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¸Ð½ÑÐµÐ³ÑÐ°ÑÐ¸Ð¸ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÐ²ÑÐ·ÐµÐ¹. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ Ð´Ð»Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð², Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐ¸ÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¾Ð¹ Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸ÐµÐ¼ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼.
title: An Analysis of Traffic Sign Performance for the Establishment of a Maintenance Plan
Creators: name: Boggs, Wesley Bill
Publisher: name: Utah State University
Year: 2012

description: Since the establishment of the first minimum retroreflectivity levels in 1993, agencies and researchers have focused on determining the service life of different sheeting type and color combinations. While deterioration curves and measured retroreflectivity are viable methods for maintaining retroreflectivity compliance, they do not ensure the ability of the traffic sign to convey its intended message. Retroreflectivity efficiency only ensures visibility but does not properly describe the legibility of the sign. Therefore, while agencies across the nation are developing and implementing traffic sign maintenance plans, the emphasis should not be solely placed on visibility.
In order to evaluate the performance of UDOT’s traffic signs, a sample sign population was collected across all four of UDOT’s maintenance regions. Analysis on this sample set not only determined the current rate of compliance, but it also identified several issues seen throughout the population. Signs under UDOT’s jurisdiction are four times more likely to have substantial damage to the sign face than to fail to meet the minimum retroreflectivity levels. Analysis was conducted on determining contributing factors damage rates and it was determined that precipitation, elevation, seasonal temperature swing, and exposure of the sign all contributed to higher rates of damage. Additional analysis was conducted on determining the service life of different type and sheeting combinations. Hindered by the lack of known installation information, the analysis only identified service life as a significant contributor to sheeting deterioration.
Since the majority of new sign installations are prismatic sheeting, the recommended maintenance plan needs to reflect the performance characteristics of this sheeting while continuing to manage the existing sign population. With the combination of UDOT’s current sign knowledge and the sheeting deterioration and damage analysis conducted in this thesis, the feasibility of the five preapproved FHWA methods is discussed. This report concludes with the recommendation of a visual nighttime inspection method due to this method’s ability to assess both the visibility and legibility of traffic signs. This will ensure that UDOT maintains compliance with the retroreflectivity mandate, while improving safety for motorists.
L’architetto cosmico
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Uno studio su un campione di oltre 3000 galassie ellittiche suggerisce l'esistenza di una relazione ben precisa tra la massa dell'alone galattico di materia oscura e quella del buco nero centrale. Questi risultati, che saranno pubblicati su Astrophysical Journal, permettono di risolvere alcune controversie in questo campo dell'astrofisica e forniscono nuovi indizi sui processi evolutivi delle galassie
Boolean networks with reliable dynamics
Creators: name: Peixoto, Tiago P.
name: Drossel, Barbara
Publisher: name: arXiv
Year: 2009
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Quantitative Methods (q-bio.QM)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: We investigated the properties of Boolean networks that follow a given reliable trajectory in state space. A reliable trajectory is defined as a sequence of states which is independent of the order in which the nodes are updated. We explored numerically the topology, the update functions, and the state space structure of these networks, which we constructed using a minimum number of links and the simplest update functions. We found that the clustering coefficient is larger than in random networks, and that the probability distribution of three-node motifs is similar to that found in gene regulation networks. Among the update functions, only a subset of all possible functions occur, and they can be classified according to their probability. More homogeneous functions occur more often, leading to a dominance of canalyzing functions. Finally, we studied the entire state space of the networks. We observed that with increasing systems size, fixed points become more dominant, moving the networks close to the frozen phase.
description: 11 Pages, 15 figures
Additional file 2: of LAPTM4B is a novel diagnostic and prognostic marker for lung adenocarcinoma and associated with mutant EGFR
Creators: name: Wang, Lu
name: Meng, Yue
name: Zhang, Qing-Yun
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Virology

description: Table S2. The sequence for RT-PCR primers and siRNAs. (DOCX 15 kb)
Ein gründliches Für und Wider die alten und neuen Textvarianten des Apostolischen Glaubensbekenntnisses
Creators: name: Junker, Thomas
Publisher: name: Lutherische Beiträge
Year: 1970

description: Lutherische Beiträge, Bd. 18 Nr. 2 (2013): Lutherische Beiträge, Band 18, Heft 2
Spuntano le piccole lune di Plutone
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2015

A 85 anni esatti dalla scoperta di Plutone, la sonda NASA New Horizons, in viaggio verso il pianeta nano, ha dato la prima occhiata prolungata alla piccola luna Hydra, la più esterna del sistema, e visto per la prima volta l’altrettanto piccola Nix
title: Analytical Modelling of the Effect of In-Depth Radiation within a Liquid Layer in the Case of a Pool Fire
Creators: name: Beji, T.
name: Merci, B.
name: International Seminar On Fire And Explosion Hazards (9; 2019; Saint Petersburg, Russia)
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: 2019

description: In this paper, we present a âsimplifiedâ approach for the numerical modelling of the convective currents
that occur within a liquid fuel in the case of a pool fire and which are induced by in-depth thermal
radiation. This approach is based on the concept of âeffectiveâ thermal conductivity, which is calculated
herein based on the analytical solution of a steady-state one-dimensional heat conduction equation
including a source term for in-depth radiation. This solution leads to a temperature profile which displays
a horizontal liquid layer (of a given depth) that is bounded by a temperature that is higher at its bottom
than its top. This thermal structure generates Rayleigh-BÃ©nard instabilities which enhance heat transfer
within the liquid. This effect is modeled via an increase of the âactualâ thermal conductivity of the liquid
by a dimensionless heat transfer number, namely the Nusselt number. The Nusselt number is calculated
based on the âclassical expressionâ of the Rayleigh number for the case of a âhorizontal cavity heated
from belowâ. The paper provides the details of the derived solution for the âeffectiveâ thermal
conductivity along with examples of application to several fuels.
title: The Impact of Different Play Environments on the Social Interactions of Toddlers with Disabilities
Creators: name: Buckley, Rebecca
Publisher: name: Utah State University
Year: 2011

description: Play is an important part of supporting social interactions with children, and these interactions are an imperative part of a child’s social development. Social development is a significant challenge for children with disabilities, making play an important component in helping with their development. Different play environments may be better than others in terms of supporting social interactions. In order to determine what types of play environments were best at supporting social interaction, children between 33 and 36 months of age were observed in three different settings. Children that were part of the Lil’ Aggies program—an early intervention program that helps children under the age of 3 with disabilities transition into community and district preschools—were observed on the playground, in the classroom, and in the gym. The social interactions in each of these environments were compared to see if one environment promoted more social interactions than another. A time-sampling procedure was used for the observations in each of the settings. Following the observations, the data were analyzed using an independent sample t-test procedure. It was found that children are more likely to interact with peers on the playground, and more likely to interact with adults in the classroom. It was also found that interactions on the playground were more likely to be positive.
title: ÐÐ»Ð¸ÑÐ½Ð¸Ðµ ÑÑÐ¾Ñ Ð°ÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð·Ð±ÑÐ¾ÑÐ° Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÑ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð¿ÑÐ¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð³Ð¸Ð´ÑÐ¾Ð¿Ð½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð° ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾Ð²Ð¾ÑÐ¾ÑÐ° ÑÐºÐ·Ð¾ÑÐºÐµÐ»ÐµÑÐ½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°
title: The influence of stochastic variation of some factors in the modeling of hydro-pneumatic drive system of rotation of an exoskeleton device
Creators: name: ÐÐ¾ÑÐ¾Ð±ÑÐµÐ²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
name: ÐÐµÑÑÐ¾Ð¿ÑÐ½, ÐÑÑÐµÐ½
name: "ÐÐ¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ, Ð³Ð¸Ð´ÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ Ð¸ Ð³Ð¸Ð´ÑÐ¾Ð¿Ð½ÐµÐ²Ð¼Ð¾Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÐºÐ°. Ð¡Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð¾-ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2020; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2020
Subjects: ÐÐ½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ

description: ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð½Ð°ÑÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Ð¸ ÑÐ°Ð±Ð¾Ñ, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð½ÑÑ Ð¿Ð¾ ÑÐºÐ·Ð¾ÑÐºÐµÐ»ÐµÑÐ½Ð¾Ð¹ ÑÐµÐ¼Ð°ÑÐ¸ÐºÐµ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð½ÑÐµ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð´Ð°Ð½Ð½ÑÑ ÑÑÑÑÐ¾Ð¹ÑÑÐ² (Ð¾ÑÑÑÑÑÑÐ²Ð¸Ðµ ÐºÐ¾Ð¼Ð¿Ð°ÐºÑÐ½ÑÑ Ð¸ Ð¼Ð¾ÑÐ½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ; Ð¿ÑÐ¾ÑÐ½ÑÐµ Ð¸ Ð»ÑÐ³ÐºÐ¸Ðµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸; Ð½Ð¸Ð·ÐºÐ°Ñ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ¾-Ð¿ÑÐ¸Ð²Ð¾Ð´Ð½Ð¾Ð¹ ÑÐ°ÑÑÐ¸; ÑÐ»Ð¾Ð¶Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ; Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ñ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ¾Ð¼), ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¾Ð±ÑÑÐ»Ð°Ð²Ð»Ð¸Ð²Ð°ÑÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¸ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº ÑÐ¸ÑÑÐµÐ¼ Ð¸ÑÐ¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¾Ð² ÑÐºÐ·Ð¾ÑÐºÐµÐ»ÐµÑÐ¾Ð². Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÐµÑÐµÑÐ¾Ð´Ð½ÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÑ, Ñ ÑÑÑÑÐ¾Ð¼ ÑÐ°Ð·Ð±ÑÐ¾ÑÐ° ÑÑÐ¾ÑÐ°ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð².
description: After the research and development papers on exoskeletons were analyzed, the following principal problem domains have been discovered: no
compact and high-capacity power supply units; no durable and light-weight designs; low energy efficiency of mechanics and actuators; complicated control system; insufficient operational safety. These problems call for additional research and development to improve functional and operating characteristics of exoskeleton actuator systems. The main transients were calculated and constructed considering variations of stochastic parameters.
Quando una stella passò nel Sistema Solare
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2015

Scoperta la stella che ci è passata più vicina: si chiama stella di Scholz, una nana rossa di piccola stazza accompagnata da una nana bruna. 70.000 anni fa si è infilata dritta nella parte esterna della Nube di Oort, il guscio di comete che rappresenta il confine estremo del Sistema Solare
title: PR-ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð² ÑÑÐµÑÐµ ÐºÑÐ»ÑÑÑÑÑ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¼ÑÐ·Ð¸ÐºÐ»Ð° Â«ÐÐ°ÑÑÐµÑ Ð¸ ÐÐ°ÑÐ³Ð°ÑÐ¸ÑÐ°Â»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»Ð¿Ð°ÐºÐ¾Ð² , ÐÑÐ¸Ð³Ð¾ÑÐ¸Ð¹
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°Ð½Ð°Ð»Ð¸Ð·
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ
Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ
analysis
organization
promotion

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° PR- ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ñ ÑÐµÐ°ÑÑÐ¾Ð² Ð² Ð Ð¾ÑÑÐ¸Ð¸. ÐÐµÑÐ¾Ð´Ð°Ð¼, Ð°Ð½Ð°Ð»Ð¸Ð·Ð°Ð¼, Ð¾Ð±Ð¾Ð±ÑÐµÐ½Ð¸Ñ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð´Ð°Ð½Ð½ÑÑ. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð³Ð»Ð°Ð²Ð½Ð¾Ð³Ð¾ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ° Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»ÐµÐ¹ PR- ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸.
description: This work is dedicated to PR strategy of the maintenance of theatres in Russia. Methods, analysis, generalization and systematization of the received data. Analyzed the content and technology of optimum planning of communication campaigns as the main tool for achieving the goals of the PR campaign.
Il lampo gamma che nasce dall’ipernova
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

E' stata la tremenda esplosione di una stella almeno 30 più massiccia del nostro Sole, avvenuta in una galassia nana, a generare il prolungato lampo di raggi Gamma (GRB) registrato il 2 luglio del 2013. La conferma arriva dallo studio condotto da un team in gran parte composto da astronomi dell’INAF, che sono riusciti a caratterizzare in dettaglio le caratteristiche della stella progenitrice e l’energia rilasciata nel cataclisma cosmico
Novae: fabbriche di Litio nell’Universo
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Più Litio del previsto nell'esplosione di una nova. E' quanto riscontrato da un team di astronomi del National Astronomical Observatory of Japan, dell'Università Osaka Kyoiku, dell'Università di Nagoya University, e dell'Università di Kyoto Sangyo che ha condotto uno studio approfondito sulla Nova Delphini 2013. Il commento di Ulisse Munari dell'INAF-Osservatorio Astronomico di Padova
La nana bruna che manca all’appello
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

La stella avrebbe dovuto essere in orbita intorno all'insolita coppia di stelle V471 Tauri. Lo strumento montato sul VLT ha registrato la sorprendente assenza e quindi lo strano comportamento di V471 Tauri deve avere un'altra spiegazione
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ð¹ ÑÑÐµÐ´Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¥Ð°Ð½ÑÑ-ÐÐ°Ð½ÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ¸Ð»Ð¸Ð°Ð»Ð° ÐÐÐ Â«Ð Ð¾ÑÑÐµÐ»ÐµÐºÐ¾Ð¼Â»)
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Ð°ÑÐ»Ð°ÐºÐ¾Ð²Ð°, ÐÐ°Ñ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: Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð°Ñ ÑÑÐµÐ´Ð°
ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÑ
swot- Ð°Ð½Ð°Ð»Ð¸Ð·
Ð¾ÑÐ´ÐµÐ» Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð°

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 Ð¾ÑÑÐµÐ»ÐµÐºÐ¾Ð¼Â».
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Family influence on child protection cases at the point of apprehension and in later foster care : an exploratory study of a group of wards (of the Children's Aid Society, Vancouver) in foster care more than two years
Creators: name: Tuckey, Elizabeth Ursula Townsend
Publisher: name: University of British Columbia
Year: 2012

description: The purpose of this study is to explore the relationship of the foster child to his own family, and to examine the resulting effects upon the child's adjustment in foster care. The goal of the child welfare worker has changed in the past twenty-five years from the provision of food, clothing, and a roof over the head of the foster child, to an attempt to meet the emotional and psychological as well as physical needs of the child. These needs are likely to vary according to the degree of deprivation suffered by the child before placement. Regardless of the inadequacy of his parents, the child has to think well of them, so far as he is able, if he is also to think well of himself. He must resolve the trauma inevitably resulting from the separation from his parents before he can settle down in his foster home, and take on new ties. Against these concepts as background, the present study examines the circumstances of thirty-four, wards of the Children's Aid Society of Vancouver, B. C., beginning with the family situation at the time of the child's removal, and covering a significant period of foster care. Part of the methodology of the study is an attempt to assess the parents’ strengths and weaknesses including their capacity for parenthood. The children are reviewed twice: once at the time of their removal from their own homes, and again at a fixed date, when all the children had been in foster care for at least two years. The degree of contact with the natural parents is kept in the focus of the study throughout. The study concludes with an assessment of some of the ways in which the foster child can be helped to accept his past, and move on to the future free from hampering or neurotic ties. The implications relate to (a) the children, (b) the natural parents, (c) the foster parents.
Die Aufgabe der Kirche angesichts von Entchristlichung, Entkirchlichung und neuen religiösen Bewegungen
Creators: name: Roth, Michael
Publisher: name: Lutherische Beiträge
Year: 1970

description: Lutherische Beiträge, Bd. 18 Nr. 2 (2013): Lutherische Beiträge, Band 18, Heft 2
title: ÐÑÐµÐµÐ¼ÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑ Ð¸Ð´ÐµÐ¹ Ð½Ð°ÑÑÐ½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐºÐ¾Ð»Ñ Ð¡. Ð¤. Ð¨Ð°ÑÐ¸Ð»Ð¾Ð²Ð° Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÐºÐ°ÑÐµÐ´Ñ Ð¸ Ð²ÑÐ·Ð¾Ð²
title: The ideas continuity of S. F. Shatilovâs scientific and methodological school in the conditions of departments and universities interaction
Creators: name: Ð¢ÑÑÐ±Ð¸ÑÐ¸Ð½Ð°, ÐÐ»ÑÐ³Ð°
name: ÐÐ¸ÑÐ¾Ð², ÐÐ°Ð»ÐµÑÐ¸Ð¹
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ

description: Ð ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð²ÑÐµ Ð±Ð¾Ð»ÑÑÐµÐµ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ ÑÐ´ÐµÐ»ÑÐµÑÑÑ Ð¾ÑÐ¼ÑÑÐ»ÐµÐ½Ð¸Ñ Ð¾Ð¿ÑÑÐ° Ð½Ð°ÑÑÐ½ÑÑ ÑÐºÐ¾Ð», Ð° Ð½Ð°Ð¸Ð±Ð¾Ð»ÑÑÐ¸Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð²Ð¾ Ð²ÑÐµÐ¼, Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ, Ð² Ð½Ð°ÑÑÐ½Ð¾Ð¼ Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¸ Ð¼Ð¾Ð¶Ð½Ð¾ Ð´Ð¾Ð±Ð¸ÑÑÑÑ ÑÐ¾Ð»ÑÐºÐ¾ Ð±Ð»Ð°Ð³Ð¾Ð´Ð°ÑÑ ÑÐ¾Ð²Ð¼ÐµÑÑÐ½ÑÐ¼ ÑÑÐ¸Ð»Ð¸ÑÐ¼.
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¸ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° ÑÑÐ°Ð½ÑÑÐ·ÑÐºÐ¾Ð¹ ÐºÑÑ Ð½Ð¸ Ð½Ð° 100 Ð¼ÐµÑÑ Ð² Ð¦ÐµÐ½ÑÑÐ°Ð»ÑÐ½Ð¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÐµÐ´Ð¾Ð²Ð°, ÐÐ°Ñ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¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
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description: ÐÑ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 ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° Ñ ÑÑÐ°Ð½ÑÑÐ·ÑÐºÐ¾Ð¹ ÐºÑÑÐ½ÐµÐ¹ Ð² Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð¿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. 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, ÐµÐ³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸.
Suzaku observation of the Phoenix Galaxy
Creators: name: Matt, G.
name: Bianchi, S.
name: Awaki, H.
name: Comastri, A.
name: Guainazzi, M.
name: Iwasawa, K.
name: Jimenez-Bailon, E.
name: Nicastro, F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In recent years, several Seyfert 2 galaxies have been discovered that change state when observed in X-rays a few years apart, switching from Compton-thin to reflection-dominated or viceversa. We observed a member of this class of "Changing-look" sources, the Phoenix Galaxy, with Suzaku, with the aim of better understanding the nature of the variations. The Suzaku spectrum was analyzed, and the results compared with previous ASCA and XMM-Newton observations. The source was caught in a Compton-thin state, as in XMM-Newton, but differently from ASCA. Comparing the Suzaku and XMM-Newton observations, a variation in the column density of the absorber on a time scale of years is discovered. A similar change, but on much shorter time scales (i.e. ks) may also explain the count-rate variations during the Suzaku observations. A soft excess is also present, likely due to continuum and line emission from photoionized circumnuclear matter.
description: Accepted for publication in Astronomy & Astrophysics
title: Ð Ð°Ð·Ð²Ð¸ÑÐ¸Ðµ ÑÐ¾Ð²Ð°ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÐµÐ³Ð¾ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÐ¸Ð¼Ð¾Ð², ÐÐ°ÑÐ°Ð½Ð°Ð³Ð°
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: Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸
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