cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð² ÑÐµÐ¾ÑÐ¸Ñ Ð´ÐµÑÐµÐºÑÐ¾Ð². Ð§. 1, Ð¢Ð¾ÑÐµÑÐ½ÑÐµ Ð´ÐµÑÐµÐºÑÑ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÑÐºÐ¸Ð½, ÐÐ¸ÑÐ°Ð¸Ð»
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2010
Subjects: ÐÑÐ¸ÑÑÐ°Ð»Ð»Ñ

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 150700 Â«Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸ÐµÂ». Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¾ Ð½Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ ÑÐµÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÑÑÑÐºÑÑÑÐµ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐ» Ð¸ Ð¾Ð± Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¸ ÑÑÐ¾Ð¹ ÑÑÑÑÐºÑÑÑÑ Ð¿Ð¾Ð´ Ð²Ð»Ð¸ÑÐ½Ð¸ÐµÐ¼ Ð²Ð½ÐµÑÐ½Ð¸Ñ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹. ÐÐ°ÑÑÑÑ Ð¾Ð±ÑÐ°Ñ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð¸ ÐºÑÐ°ÑÐºÐ¸Ð¹ Ð¾Ð±Ð·Ð¾Ñ Ð´ÐµÑÐµÐºÑÐ¾Ð² Ð² ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð°Ñ. ÐÐ·Ð»Ð°Ð³Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ¾ÑÐ¸Ð¸ ÑÐ¾ÑÐµÑÐ½ÑÑ Ð´ÐµÑÐµÐºÑÐ¾Ð². ÐÐ±ÑÐ¸Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¸Ð»Ð»ÑÑÑÑÐ¸ÑÑÑÑÑÑ ÐºÐ¾Ð½ÐºÑÐµÑÐ½ÑÐ¼Ð¸ Ð¿ÑÐ¸Ð¼ÐµÑÐ°Ð¼Ð¸ Ð¸ Ð¿ÑÐ¾ÑÑÑÐ¼Ð¸ ÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÐ¼Ð¸ Ð¾ÑÐµÐ½ÐºÐ°Ð¼Ð¸. ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð¿Ð¿Ð°ÑÐ°Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ Ð² ÑÑÐµÐ·Ð°Ð½Ð½Ð¾Ð¼ Ð²Ð¸Ð´Ðµ, Ð³ÑÐ¾Ð¼Ð¾Ð·Ð´ÐºÐ¸Ðµ Ð²ÑÐºÐ»Ð°Ð´ÐºÐ¸ Ð¾ÑÐ½Ð¾ÑÑÑÑÑ Ð½Ð° ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð². ÐÑÐµÐ´Ð¿Ð¾ÑÑÐµÐ½Ð¸Ðµ Ð¾ÑÐ´Ð°ÐµÑÑÑ ÐºÐ°ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ñ ÑÑÑÐ¾ÑÐ²ÑÐ¸ÑÑÑ Ð¼Ð¾Ð´ÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹, ÑÐ¾ÑÐ¾ÑÐ¾ Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ¶Ð´ÐµÐ½Ð½ÑÑ Ð½Ð° ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐµ. Ð ÑÐ¾ Ð¶Ðµ Ð²ÑÐµÐ¼Ñ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½ ÑÑÐ´ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð², ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¾Ð±ÑÑÐ½Ð¾ Ð½Ðµ Ð¸Ð·Ð»Ð°Ð³Ð°ÑÑÑÑ Ð² Ð¿Ð¾Ð´Ð¾Ð±Ð½ÑÑ ÐºÑÑÑÐ°Ñ, Ð½Ð¾ Ð¾ÐºÐ°Ð·ÑÐ²Ð°ÑÑÑÑ ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½Ð¾ Ð²Ð°Ð¶Ð½ÑÐ¼Ð¸ ÐºÐ°Ðº Ð´Ð»Ñ Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð´ÐµÑÐµÐºÑÐ½ÑÑ ÑÑÑÑÐºÑÑÑ, ÑÐ°Ðº Ð¸ Ð´Ð»Ñ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¸ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÑÐµÑÑÐµÐ³Ð¾ ÐºÑÑÑÐ°, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 150700 Â«Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸ÐµÂ».
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Ecco la foto della prima cometa interstellare
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2019

Nella notte tra il 9 e il 10 settembre, il Gemini North Telescope a Maunakea ha immortalato la prima cometa interstellare che sta entrando nel Sistema solare interno, C/2019 Q4 (Borisov). Attualmente, data la sua posizione in cielo, è di difficile osservazione, ma il suo percorso iperbolico la porterà a condizioni di osservazione più favorevoli nei prossimi mesi
Circulating non-coding RNAs as a tool for liquid biopsy in solid tumors
Creators: name: Dogan, Beyza Karaca
name: Yilmaz, Seda Salman
name: Izgi, Gizem Nur
name: Ozen, Mustafa
Publisher: name: Taylor & Francis
Year: 2025
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Mental Health

description: Solid tumors are significant causes of global mortality and morbidity. Recent research has primarily concentrated on finding pathology-specific molecules that can be acquired non-invasively and that can change as the disease progresses or in response to treatment. The focus of research has moved to RNA molecules that are either freely circulating in body fluids or bundled in microvesicles and exosomes because of their great stability in challenging environments, ease of accessibility, and changes in level in response to therapy. In this context, there are many non-coding RNAs that can be used for this purpose in liquid biopsies. Out of these, microRNAs have been extensively studied. However, there has been an increase of interest in studying long non-coding RNAs, piwi interacting RNAs, circular RNAs, and other small non-coding RNAs. In this article, an overview of the most researched circulating non-coding RNAs in solid tumors will be reviewed, along with a discussion of the significance of these molecules for early diagnosis, prognosis, and therapeutic targets. The publications analyzed were extracted from the PubMed database between 2008 and June 2024. RNAs that will not translate to proteins are called non-coding RNAs. These small molecules are still mystery of the human genetics and significantly associated with cancer. Their diverse functions, along with their potential to early diagnose cancer and monitor cancer development, warrant further consideration and investigation. In this article, the role of these small molecules in early diagnosing, monitoring and therapy development in solid cancer types are being discussed.
The Sloan Nearby Cluster Weak Lensing Survey
Creators: name: Kubo, Jeffrey M.
name: Annis, James
name: Hardin, Frances Mei
name: Kubik, Donna
name: Lawhorn, Kelsey
name: Lin, Huan
name: Nicklaus, Liana
name: Nelson, Dylan
name: Reis, Ribamar R. R.
name: Seo, Hee-Jong
name: Soares-Santos, Marcelle
name: Stebbins, Albert
name: Yunker, Tony
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We describe and present initial results of a weak lensing survey of nearby ($\rm{z}\lesssim0.1$) galaxy clusters in the Sloan Digital Sky Survey (SDSS). In this first study, galaxy clusters are selected from the SDSS spectroscopic galaxy cluster catalogs of \citet{miller05} and \citet{berlind06}. We report a total of seven individual low redshift cluster weak lensing measurements which include: A2048, A1767, A2244, A1066, A2199, and two clusters specifically identified with the C4 algorithm. Our program of weak lensing of nearby galaxy clusters in the SDSS will eventually reach $\sim 200$ clusters, making it the largest weak lensing survey of individual galaxy clusters to date.
description: accepted to ApJL; 11 pages, 1 figure
title: Fallgeschichten der Psychoanalyse
Creators: name: Harst, Joachim
Publisher: name: Graduate School Practices of Literature
Year: 2023
Subjects: subject: 800 Literature (Belles-lettres) and rhetoric

description: Der Aufsatz beschäftigt sich mit der Bedeutung der »Fallgeschichte« in der psychoanalytischen Therapie und Theorie. Dabei changiert die Bedeutung des »Falls« jedoch zwischen verschiedenen Registern, unter denen hier »casus«, »Rätsel« und »lapsus« diskutiert werden. Sie werden anhand von Freuds »Bruchstück einer Hysterie-Analyse« erläutert, wobei ein besonderes Augenmerk auf unterschiedliche mediale Konstellationen gelegt wird, die dazu dienen sollen, der Mehrdeutigkeit des Falls Herr zu werden.
Corona lunare per Giorgia Hofer
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2019

A due settimane esatte dalla sua “Congiunzione ad alta quota”, un’altra opera dell’astrofotografa di Valle di Cadore viene scelta dalla Nasa come immagine astronomica del giorno: una particolarissima immagine della Luna sulla città della Mole, scattata in occasione di una visita all’Osservatorio astrofisico dell’Inaf di Torino
title: ÐÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³Ð¸Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÑÑÐ¾Ð²Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
name: ÐÐ°ÑÐ¸Ð»ÑÐµÐ²Ð°, ÐÐ»ÑÐ³Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2012
Subjects: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸
Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð´ÑÑÐ°Ð½ÑÐ¸Ð¸

description: ÐÐ·Ð»Ð°Ð³Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ, ÑÐµÑÐ°ÐµÐ¼ÑÐµ Ð¿ÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÑÐ°Ð½ÑÐ¸Ð¹ Ð¸ Ð¿Ð¾Ð´ÑÑÐ°Ð½ÑÐ¸Ð¹: Ð²ÑÐ±Ð¾Ñ Ð³Ð»Ð°Ð²Ð½ÑÑ ÑÑÐµÐ¼ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹, ÑÐ°ÑÑÐµÑ ÑÐ¾ÐºÐ¾Ð² ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ, Ð²ÑÐ±Ð¾Ñ ÐºÐ¾Ð¼Ð¼ÑÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ¾Ð², ÑÐ¸Ð½, ÑÐ¾ÐºÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¾Ð², ÐºÐ°Ð±ÐµÐ»ÐµÐ¹, ÑÐ¾ÐºÐ¾Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐ¸Ð²Ð°ÑÑÐ¸Ñ ÑÐµÐ°ÐºÑÐ¾ÑÐ¾Ð², Ð²ÑÐ±Ð¾Ñ Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÑ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ¾Ð² ÑÐ¾ÐºÐ° Ð¸ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ, Ð¾ÑÐ½Ð¾Ð²Ñ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð² ÑÐ»ÐµÐºÑÑÐ¾ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ°Ñ. ÐÐ°ÑÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐµÑÑÐµÐ¶ÐµÐ¹ Ð³Ð»Ð°Ð²Ð½Ð¾Ð¹ ÑÑÐµÐ¼Ñ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÑÑÑÐ¾Ð¹ÑÑÐ². ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½ Ð² Ð²Ð¸Ð´Ðµ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð¿Ð¾ Ð½Ð¾Ð²ÑÐ¼ ÑÐ¸Ð¿Ð°Ð¼ ÐºÐ¾Ð¼Ð¼ÑÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ¾Ð², ÑÐ¸Ð½Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¾Ð², ÐºÐ°Ð±ÐµÐ»ÐµÐ¹, Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¼ ÑÐ¸ÑÑÐµÐ¼Ð°Ð¼ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ»ÐµÐºÑÑÐ¾Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ âÐ­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ°â, Ð²ÑÐ¿Ð¾Ð»Ð½ÑÑÑÐ¸Ñ ÐºÑÑÂ­ÑÐ¾Ð²Ð¾Ð¹ Ð¿ÑÐ¾ÐµÐºÑ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ âÐÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³Ð¸Ð¸â Ð¸ Ð²ÑÐ¿ÑÑÐºÐ½ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÑÑ ÑÐ°Ð±Ð¾ÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð´ÑÑÐ³Ð¸Ñ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ¾Ð², Ð²ÑÐ¿Ð¾Ð»Ð½ÑÑÑÐ¸Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ðµ ÐºÑÑÑÐ¾Ð²ÑÐµ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð¸ ÑÐ°Ð±Ð¾ÑÑ. ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð² Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¸Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¹.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Pesata la madre di tutte le pulsar
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2019

Utilizzando come “bilancia” un fenomeno relativistico detto “ritardo di Shapiro”, un team di astronomi guidato da H. Thankful Cromartie della University of Virginia ha individuato la stella di neutroni più massiccia a oggi conosciuta: è pari a circa 2.14 masse solari
One loop renormalizability of the Poisson-Lie sigma models
Creators: name: Valent, G.
name: Klimcik, C.
name: Squellari, R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present the proof of the one loop renormalizability in the strict field theoretic sense of the Poisson-Lie sigma models. The result is valid for any Drinfeld double and it relies solely on the Poisson-Lie structure encoded in the target manifold.
description: 11 pages
Sentita l’armonia delle onde gravitazionali
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2019

Ascoltando toni specifici nelle onde gravitazionali generate dalla fusione di buchi neri, i ricercatori stanno mettendo alla prova la teoria di Einstein. In particolare, sono riusciti a sentire due ipertoni, suoni armonici la cui frequenza è multipla del suono fondamentale, in un evento che ha portato alla formazione di un buco nero, scoprendo che gli ipertoni sono rilevabili prima che il suono principale diventi visibile
Spin foam models for quantum gravity from lattice path integrals
Creators: name: Bonzom, Valentin
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Spin foam models for quantum gravity are derived from lattice path integrals. The setting involves variables from both lattice BF theory and Regge calculus. The action consists in a Regge action, which depends on areas, dihedral angles and includes the Immirzi parameter. In addition, a measure is inserted to ensure a consistent gluing of simplices, so that the amplitude is dominated by configurations which satisfy the parallel transport relations. We explicitly compute the path integral as a sum over spin foams for a generic measure. The Freidel-Krasnov and Engle-Pereira-Rovelli models correspond to a special choice of gluing. In this case, the equations of motion describe genuine geometries, where the constraints of area-angle Regge calculus are satisfied. Furthermore, the Immirzi parameter drops out of the on-shell action, and stationarity with respect to area variations requires spacetime geometry to be flat.
description: 19 pages, 1 figure
Il cosmo e l’uomo nella storia
Creators: Giuseppe Fiasconaro
Publisher: name: Media Inaf
Year: 2019

Dal 18 al 20 settembre, un confronto fra studiosi di diverse aree disciplinari – dalla fisica all’antropologia culturale, dalla storia delle religioni e delle tradizioni popolari alla sociologia – per analizzare la complessa trama di relazioni che lega la cosmologia scientifica e le concezioni “cosmiche” elaborate sia dalle culture antiche e folkloriche sia dalle società contemporanee. Ne parliamo con Antonino La Barbera dell’Inaf-Iasf di Palermo
Can non-open data standards legally taint conforming codebases and databanks?
Creators: name: Morrison, Robbie
Publisher: name: Zenodo
Year: 2023
Subjects: open data
semantic standards
derivative works
energy system modeling

description: This presentation examines whether systems modeling artifacts — like modeling frameworks, high‑resolution databanks, and scenarios databases — might become derivative works of their informing semantic standards. And if so, would the use of proprietary standards then taint the open science status of these artifacts in the process. A diagram outlining this proposition is provided on slide 25.
description: This release with minor post‑presentation improvements and updated CC0-1.0 question.
APPLICATION OF FATTY ACID FOR PHARMACEUTICALS
Creators: name: Takron Chantadee
name: Nutdanai Lertsuphovanit
name: Thawatchai Phaechamud
Publisher: name: Faculty of pharmacy, Silpakorn University
Year: 2019
Subjects: fatty acid
application
pharmaceuticals

description: Thai Bulletin of Pharmaceutical Sciences, 14, 1(January-December)2019, 1-11
title: ÐÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ° Ð¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑ Ð½Ð¸ÐºÐ°. ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Visual Fortran
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÐ¼ÐµÑÐ¾Ð²Ð°, ÐÐ°ÑÑÐ»Ð»Ð°
name: ÐÐ°ÑÐ¿Ð¾Ð²Ð°, ÐÑÐ¸Ð½Ð°
name: Ð¢Ð¸ÑÐºÐ¾Ð², ÐÐ°ÑÐ¸Ð»Ð¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£
Year: 2002
Subjects: Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ°
Ð­Ð»ÐµÐºÑÑÐ¾ÑÐµÑ Ð½Ð¸ÐºÐ°

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ Ð°Ð²ÑÐ¾ÑÑÐºÐ¸Ð¹ ÐºÑÑÑ, Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð½ÑÐ¹ Ð´Ð»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ 551700 Â«Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ°Â» Ð¸ 551300 Â«Ð­Ð»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐ°, ÑÐ»ÐµÐºÑÑÐ¾Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ° Ð¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÂ». ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¸ ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½ÑÐ¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð», Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐ¹ Ð´Ð»Ñ ÑÑÐ¿ÐµÑÐ½Ð¾Ð³Ð¾ Ð¾Ð²Ð»Ð°Ð´ÐµÐ½Ð¸Ñ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½ ÐÐÐ¡ 071600 Â«ÐÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ° Ð¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐ°Â», Ð² ÐºÐ¾ÑÐ¾ÑÑÑ Ð²ÐµÐ´ÑÑÑÑ ÑÐ¾Ð»Ñ Ð¸Ð³ÑÐ°ÐµÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ¾Ð² Ð¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð² ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸ Â«Ð Ð°ÑÑÐµÑ ÑÐ»ÐµÐºÑÑÐ¾Ð¼Ð°Ð³Ð½Ð¸ÑÐ½ÑÑ Ð¿Ð¾Ð»ÐµÐ¹Â», Â«ÐÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½Ð°Ñ Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ñ Ð¸ Ð¿ÐµÑÐµÐ½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸ÑÂ», Â«ÐÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½ÑÐµ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸Â», Â«ÐÐµÑÐµÑÐ¾Ð´Ð½ÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÑ Ð² ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐµÂ». Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð²ÐµÑÑÐ¸Ð¸ ÑÐ·ÑÐºÐ° ÑÐµÑÐµÐ½Ð¸Ñ Ð½Ð°ÑÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð´Ð°Ñ Ð¤Ð¾ÑÑÑÐ°Ð½ - Visual Fortran. ÐÐ°ÑÑÐ´Ñ Ñ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð¸ÐµÐ¼ Ð¾ÑÐ½Ð¾Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Visual Fortran Ð¾ÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð²ÑÐ¾Ð´ÑÑÐµÐ¹ Ð² ÐµÐ³Ð¾ ÑÐ¾ÑÑÐ°Ð² Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð´Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ (IMSL) Ð² Ð·Ð°Ð´Ð°ÑÐ°Ñ, ÑÐ°ÑÐ°ÐºÑÐµÑÐ½ÑÑ Ð´Ð»Ñ Ð½Ð°Ð·Ð²Ð°Ð½Ð½ÑÑ Ð²ÑÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¸ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½. ÐÑÐ´ÐµÐ»ÑÐ½Ð¾ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Visual Fortran Ð´Ð»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ¾Ð² Ð´Ð»Ñ Windows, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ¸Ñ ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² III-VI ÐºÑÑÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ ÑÐºÐ°Ð·Ð°Ð½Ð½ÑÐ¼ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
News planetarie da Ginevra… stay tuned
Creators: Caterina Boccato
Publisher: name: Media Inaf
Year: 2019

Si apre ufficialmente oggi in Svizzera il convegno sulle scienze planetarie con la più ampia partecipazione mondiale. Uno sforzo congiunto Europa-Usa, nello specifico tra la Europlanet Society e l’American Astronomical Society, grazie al quale i maggiori esperti di sistemi planetari, dal nostro a quelli esterni, si incontrano per discutere le ultime novità sul campo
title: ÐÐ¾Ð´Ð¾Ñ ÑÐ°Ð½Ð¸Ð»Ð¸ÑÐ½ÑÐ¹ Ð³Ð¸Ð´ÑÐ¾ÑÐ·ÐµÐ» Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÐÐ¾ÑÑÐ¾ÑÐ½Ð¾Ð¹ Ð¡Ð¸Ð±Ð¸Ñ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Ð¸ÑÑÐ¾ÑÐ¸Ð½Ð°, 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: Ð²ÑÑÐ¾ÐºÐ¾Ð½Ð°Ð¿Ð¾ÑÐ½ÑÐ¹ Ð³Ð¸Ð´ÑÐ¾ÑÐ·ÐµÐ»
ÐºÐ¾Ð¼Ð¿Ð¾Ð½Ð¾Ð²ÐºÐ°
Ð³ÑÑÐ½ÑÐ¾Ð²Ð°Ñ Ð¿Ð»Ð¾ÑÐ¸Ð½Ð°
ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ ÑÑÐ½Ð½ÐµÐ»Ñ
Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÑÐµÑ

description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð½Ð°Ñ Ð¿Ð¾Ð´ ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ²Ð¾Ð¼ Ð´Ð¾ÑÐµÐ½ÑÐ° ÐºÐ°ÑÐµÐ´ÑÑ ÐÐ¸ÐÐ¡, Ðº.Ñ.Ð½. Ð.Ð.Ð¤ÑÐ¾Ð»Ð¾Ð²Ð¾Ð¹, ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÑ Ð²ÑÑÐ¾ÐºÐ¾Ð½Ð°Ð¿Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð³Ð¸Ð´ÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð³Ð¸Ð´ÑÐ¾ÑÐ·Ð»Ð° Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÐÐ¾ÑÑÐ¾ÑÐ½Ð¾Ð¹ Ð¡Ð¸Ð±Ð¸ÑÐ¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð²Ð°ÑÐ¸Ð°Ð½Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½Ð¾Ð²ÐºÐ¸ Ð³Ð¸Ð´ÑÐ¾ÑÐ·Ð»Ð°, Ð²ÐºÐ»ÑÑÐ°ÑÑÐµÐ³Ð¾ Ð² ÑÐµÐ±Ñ Ð³ÑÑÐ½ÑÐ¾Ð²ÑÑ Ð¿Ð»Ð¾ÑÐ¸Ð½Ñ, ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ ÑÐ°ÑÑÐ½ÑÐ¹ Ð²Ð¾Ð´Ð¾ÑÐ±ÑÐ¾Ñ, Ð²Ð¾Ð´Ð¾Ð¿ÑÐ¸ÑÐ¼Ð½Ð¸Ðº Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ ÑÑÐ½Ð½ÐµÐ»ÑÐ½ÑÐ¹ Ð²Ð¾Ð´Ð¾ÑÐ±ÑÐ¾Ñ. ÐÐ»Ñ Ð·ÐµÐ¼Ð»ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ¸Ð½Ñ Ð´Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð¿ÑÐ¾ÑÐµÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° ÑÐ°Ð±Ð¾Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÑÑÐµÐ¶Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð²ÑÑÐ¾ÐºÐ¾Ð½Ð°Ð¿Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð³Ð¸Ð´ÑÐ¾ÑÐ·Ð»Ð°.
Young Brown Dwarfs in the Core of the W3 Main Star-Forming Region
Creators: name: Ojha, D. K.
name: Tamura, M.
name: Nakajima, Y.
name: Saito, H.
name: Pandey, A. K.
name: Ghosh, S. K.
name: Aoki, K.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of deep and high-resolution (FWHM ~ 0".35) JHK NIR observations with the Subaru telescope, to search for very low mass young stellar objects (YSOs) in the W3 Main star-forming region. The NIR survey covers an area of ~ 2.6 arcmin^2 with 10-sigma limiting magnitude exceeding 20 mag in the JHK bands. The survey is sensitive enough to provide unprecedented details in W3 IRS 5 region and reveals a census of the stellar population down to objects below the hydrogen-burning limit. We construct JHK color-color (CC) and J-H/J and H-K/K color-magnitude (CM) diagrams to identify very low luminosity YSOs and to estimate their masses. Based on these CC and CM diagrams, we identified a rich population of embedded YSO candidates with infrared excesses (Class I and Class II), associated with the W3 Main region. A large number of red sources (H-K > 2) have also been detected around W3 Main. We argue that these red stars are most probably pre-main-sequence (PMS) stars with intrinsic color excesses. Based on the comparison between theoretical evolutionary models of very low-mass PMS objects with the observed CM diagram, we find there exists a substantial substellar population in the observed region. The mass function (MF) does not show the presence of cutoff and sharp turnover around the substellar limit, at least at the hydrogen-burning limit. Furthermore, the MF slope indicates that the number ratio of young brown dwarfs and hydrogen-burning stars in the W3 Main is probably higher than those in Trapezium and IC 348. The presence of mass segregation, in the sense that relatively massive YSOs lie near the cluster center, is seen. The estimated dynamical evolution time indicates that the observed mass segregation in the W3 Main may be the imprint of the star formation process.
description: 39 pages, 15 figures. Accepted for publication in the Astrophysical Journal
Near-infrared/optical identification of five low-luminosity X-ray pulsators
Creators: name: Kaur, Ramanpreet
name: Wijnands, Rudy
name: Paul, Biswajit
name: Patruno, Alessandro
name: Degenaar, Nathalie
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the identification of the most likely near-infrared/optical counterparts of five low-luminosity X-ray pulsators (AX J1700.1-4157, AX 1740.1-2847, AX J1749.2-2725, AX J1820.5-1434 and AX J1832.3-0840) which have long pulse periods (> 150 s). The X-ray properties of these systems suggest that they are likely members of persistent high mass X-ray binaries or intermediate polars. Using our Chandra observations, we detected the most likely counterparts of three sources (excluding AX J1820.5-1434 and AX J1832.3-0840) in their ESO - NTT near-infrared observations, and a possible counterpart for AX J1820.5-1434 and AX J1832.3-0840 in the 2MASS and DSS observations respectively. We also performed the X-ray timing and spectral analysis for all the sources using our XMM-Newton observations, which further helped us to constrain the nature of these systems. Our multiwavelength observations suggest that AX J1749.2-2725 and AX J1820.5-1434 most likely harbor accreting neutron stars while AX J1700.1-4157, AX J1740.1-2847 and AX J1832.3-0840 could be intermediate polars.
description: 11 pages, 5 figures, Submitted to MNRAS
Modeling the System Parameters of 2M1533+3759: A New Longer-Period Low-Mass Eclipsing sdB+dM Binary
Creators: name: For, B. -Q.
name: Green, E. M.
name: Fontaine, G.
name: Drechsel, H.
name: Shaw, J. S.
name: Dittmann, J. A.
name: Fay, A. G.
name: Francoeur, M.
name: Laird, J.
name: Moriyama, E.
name: Morris, M.
name: Rodríguez-López, C.
name: Sierchio, J. M.
name: Story, S. M.
name: Strom, A.
name: Wang, C.
name: Adams, S. M.
name: Bolin, D. E.
name: Eskew, M.
name: Chayer, P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present new photometric and spectroscopic observations for 2M 1533+3759 (= NSVS 07826147). It has an orbital period of 0.16177042 day, significantly longer than the 2.3--3.0 hour periods of the other known eclipsing sdB+dM systems. Spectroscopic analysis of the hot primary yields Teff = 29230 +/- 125 K, log g = 5.58 +/- 0.03 and log N(He)/N(H) = -2.37 +/- 0.05. The sdB velocity amplitude is K1 = 71.1 +/- 1.0 km/s. The only detectable light contribution from the secondary is due to the surprisingly strong reflection effect. Light curve modeling produced several solutions corresponding to different values of the system mass ratio, q(M2/M1), but only one is consistent with a core helium burning star, q=0.301. The orbital inclination is 86.6 degree. The sdB primary mass is M1 = 0.376 +/- 0.055 Msun and its radius is R1 = 0.166 +/- 0.007 Rsun. 2M1533+3759 joins PG0911+456 (and possibly also HS2333+3927) in having an unusually low mass for an sdB star. SdB stars with masses significantly lower than the canonical value of 0.48 Msun, down to as low as 0.30 Msun, were theoretically predicted by Han et al. (2002, 2003), but observational evidence has only recently begun to confirm the existence of such stars. The existence of core helium burning stars with masses lower than 0.40--0.43 Msun implies that at least some sdB progenitors have initial main sequence masses of 1.8--2.0 Msun or more, i.e. they are at least main sequence A stars. The secondary is a main sequence M5 star.
description: 47 pages, 7 figures
Inedita Vista sulla Grande Nube di Magellano
Creators: Redazione Eso
Publisher: name: Media Inaf
Year: 2019

Il telescopio Vista dell’Eso rivela una straordinaria immagine della Grande Nube di Magellano, una delle galassie più vicine alla nostra. Vista ha osservato questa galassia e la sua cugina, la Piccola Nube di Magellano, oltre ai loro dintorni, con dettagli senza precedenti
Bromus rubens
Creators: name: Cardona, Àngel Manuel Hernández
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Bromus
Bromus rubens

description: Bromus rubens L.
(bromus rogenc). Aborigen d’Europa meridional, Àfrica septentrional i Àsia occidental i central, s’ha estès a algunes altres parts del globus. Es fa en comunitats d’herbes anuals, ermassos, pedregars i vores de camins, fins i tot en indrets àrids. Apareix bastant freqüentment en codines de les zones mitjanes i altes.
description: Published as part of Cardona, Àngel Manuel Hernández, 2022, Catàleg actualitzat i claus d'identificació de les gramínies de Sant Llorenç del Munt i l'Obac (Barcelona), pp. 64-86 in Nemus 12 on page 69, DOI: 10.5281/zenodo.12170499
title: ÐÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð½Ð° ÑÑÐ½ÐºÐµ ÑÐµÐºÐ»Ð°Ð¼Ð½ÑÑ ÑÑÐ»ÑÐ³ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐµÐ´Ð¸Ð° Ð³ÑÑÐ¿Ð¿Ð°Â»)
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ÐµÐ»ÑÐ½Ð¸ÐºÐ¾Ð²Ð°, 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: Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸
ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ
Ð¼ÐµÑÐ¾Ð´Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ
ÑÐµÐºÐ»Ð°Ð¼Ð½Ð°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
ÑÐ¸ÑÐ¼ÐµÐ½Ð½ÑÐ¹ ÑÑÐ¸Ð»Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸ Ñ ÐºÐ»Ð¸ÐµÐ½ÑÐ°Ð¼Ð¸, Ð°Ð³ÐµÐ½ÑÑÑÐ²Ð°Ð¼Ð¸, Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÑÑÐ¸Ð¼Ð¸ ÑÐ²Ð¾Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð² ÑÑÐµÑÐµ ÑÐµÐºÐ»Ð°Ð¼Ñ Ð¸ Ð±ÑÐµÐ½Ð´Ð¸Ð½Ð³Ð°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÐÐÐ Â«ÐÐµÐ´Ð¸Ð° ÐÑÑÐ¿Ð¿Ð°Â». ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸Ð¼ÐµÑÑÐ¸ÑÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð¾Ð± ÐÐÐ Â«ÐÐµÐ´Ð¸Ð° ÐÑÑÐ¿Ð¿Ð°Â», ÑÐµÐºÑÑÐµÐ¹ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¿ÑÐ¾Ð²ÐµÐ´ÑÐ½Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ. Ð Ð°Ð±Ð¾ÑÐ° ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ, ÑÑÐµÑ Ð³Ð»Ð°Ð², Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ñ Ð¸ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹.
Ponderomotive acceleration of hot electrons in tenuous plasmas
Creators: name: Geyko, V. I.
name: Fraiman, G. M.
name: Dodin, I. Y.
name: Fisch, N. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: The oscillation-center Hamiltonian is derived for a relativistic electron injected with an arbitrary momentum in a linearly polarized laser pulse propagating in tenuous plasma, assuming that the pulse length is smaller than the plasma wavelength. For hot electrons generated at collisions with ions under intense laser drive, multiple regimes of ponderomotive acceleration are identified and the laser dispersion is shown to affect the process at plasma densities down to 10^17 cm-3. Assuming a/gamma_g << 1, which prevents net acceleration of the cold plasma, it is also shown that the normalized energy gamma of hot electrons accelerated from the initial energy gamma_0
Bromus squarrosus
Creators: name: Cardona, Àngel Manuel Hernández
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Bromus
Bromus squarrosus

description: Bromus squarrosus L.
(bromus esquarrós). Es troba al sud d’Europa, nord d’Àfrica i sud-oest d’Àsia, i, com a planta introduïda, en algunes parts d’Amèrica. Creix en pastures, vessants assolellats i vores de camins, preferentment sobre sòls calcaris i nitrificats. Només ha estat referit del massís de l’Obac.
description: Published as part of Cardona, Àngel Manuel Hernández, 2022, Catàleg actualitzat i claus d'identificació de les gramínies de Sant Llorenç del Munt i l'Obac (Barcelona), pp. 64-86 in Nemus 12 on page 69, DOI: 10.5281/zenodo.12170499
Achieving Invisibility of Homogeneous Radially Anisotropic Cylinders by Effective Medium Theory
Creators: name: Ni, Yaxian
name: Gao, Lei
name: Qiu, Cheng-Wei
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: In this paper, we establish the full-wave electromagnetic scattering theory to study the electromagnetic scattering from infinitely long cylinders with radially anisotropic coatings. We show that the total effective scattering width can be dramatically reduced by the suitable adjustment of the dielectric anisotropy of the shell, while it is not the case for tuning the dielectric anisotropy of the core. Furthermore, we could make the cylindrical objects invisible when both dielectric and magnetic anisotropies are adjusted. In the long wavelength limit, we develop effective medium theory to derive the effective isotropic permittivity and permeability for the anisotropic coated cylinders, and the invisibility radius ratio derived from the full-wave theory for small coated cylinders can be well described within the effective medium theory.
description: 15 pages, 5 figures
Clessidra gigante al centro della Via Lattea
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2019

Un team internazionale di astronomi ha scoperto una delle caratteristiche più estese mai osservate prima in prossimità del centro della Via Lattea: una coppia di enormi bolle radio-emittenti che torreggiano centinaia di anni luce sopra e sotto la regione centrale della nostra galassia, come un’enorme clessidra. Tutti i dettagli su Nature
Magnetic Response of NiFe2O4 nanoparticles in polymer matrix
Creators: name: Poddar, A.
name: Bhowmik, R. N.
name: De, Amitabha
name: Sen, Pintu
Publisher: name: arXiv
Year: 2008
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report the magnetic properties of magnetic nano-composite, consisting of different quantity of NiFe2O4 nanoparticles in polymer matrix. The nanoparticles exhibited a typical magnetization blocking, which is sensitive on the variation of magnetic field, mode of zero field cooled/field cooled experiments and particle quantity in the matrix. The samples with lower particle quantity showed an upturn of magnetization down to 5 K, whereas the blocking of magnetization dominates at lower temperatures as the particle quantity increases in the polymer. We examine such magnetic behaviour in terms of the competitive magnetic ordering between core and surface spins of nanoparticles, taking into account the effect of inter-particle (dipole-dipole) interactions on nanoparticle magnetic dynamics.
description: 5 fihure
Influence of thermohaline convection on diffusion-induced iron accumulation in A stars
Creators: name: Théado, Sylvie
name: Vauclair, Sylvie
name: Alecian, Georges
name: LeBlanc, Francis
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Atomic diffusion may lead to heavy element accumulation inside stars in certain specific layers. Iron accumulation in the Z-bump opacity region has been invoked by several authors to quantitatively account for abundance anomalies observed in some stars, or to account for stellar oscillations through the induced $κ$-mechanism. These authors however never took into account the fact that such an accumulation creates an inverse $μ$-gradient, unstable for thermohaline convection. Here, we present results for A-F stars, where abundance variations are computed with and without this process. We show that iron accumulation is still present when thermohaline convection is taken into account, but much reduced compared to when this physical process is neglected. The consequences of thermohaline convection for A-type stars as well as for other types of stars are presented
description: 19 pages, 8 figures Accepted for publication in Astrophysical Journal, August 4, 2009
Quei lampi che non ti aspetti dalla pulsar
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2019

Per la prima volta, un team di ricercatori guidato da Alessandro Papitto dell’Inaf ha osservato l’emissione contemporanea di impulsi di luce visibile e raggi X proveniente da una pulsar in rapidissima rotazione
Infected gartner duct cyst
Creators: name: NicolÃ¡S Liza, Lidia
Publisher: name: EURORAD
Year: 2015
Subjects: subject: Abdomen
subject: Genital / Reproductive system female
subject: CT
subject: Diagnostic procedure
subject: Cysts
subject: Pathology

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 30 years
description: Clinical History: A 30 years-old woman presented to the emergency room with left lower quadrant pain for the last two weeks. Purulent vaginal discharge and urinary retention were added in the last 24 hours.High acute phase reactants levels and leukocytosis were found... Final Diagnosis: Infected gartner duct cyst with bicornueate uterus and renal agenesis.
title: Ð­Ð»ÐµÐºÑÑÐ¾Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ñ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ½ÑÑ Ð¿Ð»ÐµÐ½Ð¾Ðº Ð¿ÑÐ¸ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½Ð¾Ð¼ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð½Ð°Ð³ÑÑÐ¶ÐµÐ½Ð¸Ð¸
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Ð¿Ð°ÑÐµÐµÐ², ÐÐ»ÐµÐºÑÐµÐ¹
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: Ð­Ð»ÐµÐºÑÑÐ¾Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ñ
ÐÐ»ÐµÐ½ÐºÐ¸ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ½ÑÐµ
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description: ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ð¸ Ð¿Ð»ÐµÐ½Ð¾Ðº ÐÐ­Ð¢Ð¤ ÑÐ¾Ð»ÑÐ¸Ð½Ð¾Ð¹ 3 Ð¼Ð¸ÐºÑÐ¾Ð¼ÐµÑÑÐ° Ð¿ÑÐ¸ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¸ Ð½Ð° Ð½ÐµÐµ Ð²ÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½ÑÑ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ¾Ð² Ð°Ð¼Ð¿Ð»Ð¸ÑÑÐ´Ð¾Ð¹ 1700-2400 V Ð¸ Ð´Ð»Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ ÑÑÐ¾Ð½ÑÐ° 100 ns. Ð¢Ð°ÐºÐ¸Ðµ Ð¸Ð¼Ð¿ÑÐ»ÑÑÑ ÑÐ¾Ð·Ð´Ð°Ð²Ð°Ð»Ð¸ Ð² Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð¹ Ð¿Ð»ÐµÐ½ÐºÐµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð»Ñ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð½Ð¾ÑÑÑÑ 633-800 MV/m.
ÐÐ»Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÐ¿ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸, Ð² ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð½Ð°Ð±Ð»ÑÐ´Ð°Ð»Ð¾ÑÑ ÑÐ²ÐµÑÐµÐ½Ð¸Ðµ, Ð±ÑÐ» Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½ Ð½Ð°Ð±Ð¾Ñ ÑÐ²ÐµÑÐ¾ÑÐ¸Ð»ÑÑÑÐ¾Ð², ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·ÑÑÑÐ¸ÑÑÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐ¼Ð¸ Ð¿Ð¾Ð»Ð¾ÑÐ°Ð¼Ð¸ Ð¿ÑÐ¾Ð¿ÑÑÐºÐ°Ð½Ð¸Ñ ÑÐ²ÐµÑÐ°.
Caccia alla materia strana
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2019

Dopo l'esperimento E15 che ha dato ottimi risultati all’acceleratore J-Parc in Giappone con la rilevazione di uno stato legato nucleare con "stranezza", ai Laboratori nazionali di Frascati si dà la caccia a uno stato atomico in cui un kaone con carica negativa si lega con un nucleo di carica positiva generando un atomo esotico - l'atomo kaonico. Il commento di Catalina Curceanu dell’Infn, prima autrice di uno studio in proposito su Reviews of Modern Physics
title: Ð¡Ð¸Ð½Ñ ÑÐ¾Ð½Ð½Ð¾Ðµ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ. ÐÐ´Ð½Ð¾Ð¿ÐµÑÐ¸Ð¾Ð´Ð½ÑÐµ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼Ð¾Ð´ÐµÐ»Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ°ÐµÐ², ÐÐ»ÐµÐºÑÐµÐ¹
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
Subjects: ÐÐ¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÑ
ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
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ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â» Ð´Ð½ÐµÐ²Ð½Ð¾Ð¹ Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ»ÑÑÐ°ÑÐµÐ»ÑÐ¼ Ð¿Ð¾ Ð²ÑÐ¾ÑÐ¾Ð¼Ñ Ð²ÑÑÑÐµÐ¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ½Ð¾ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ ÑÐ°ÐºÐ¶Ðµ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ Ð´ÑÑÐ³Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ.
Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾Ð´Ð½Ð¾Ð¿ÐµÑÐ¸Ð¾Ð´Ð½ÑÐµ Ð¼Ð¾Ð´ÐµÐ»Ð¸, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÐµ Ð² Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÐµÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð² ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸ Ð¼Ð¾Ð´ÐµÐ»Ñ ÐÐ»ÑÐ±Ð°ÑÐ°.
Risolto il giallo della dicotomia di Oosterhoff
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2019

Ha tenuto impegnati gli astronomi per oltre ottant’anni. Ora, grazie al più grande catalogo in assoluto di RR Lyrae – con misure spettroscopiche della metallicità per quasi 3000 stelle – un team di astronomi guidato da Michele Fabrizio, ricercatore postdoc all’Inaf di Roma e a Ssdc-Asi, è venuto a capo del problema
Open Source Portable Photodetection Platform (OS3P)
Creators: name: Kerestes, Ondrej
name: Pohanka, Miroslav
Publisher: name: Open Science Framework
Year: 2022
Subjects: subject: Pharmacology, Toxicology and Environmental Health
subject: Chemistry
subject: Biochemistry, Biophysics, and Structural Biology
subject: Engineering
subject: Biomedical Engineering and Bioengineering
subject: Biochemistry
subject: Analytical Chemistry
subject: FOS: Chemical sciences
subject: Physical Sciences and Mathematics
subject: Other Pharmacology, Toxicology and Environmental Health
subject: Biomedical Devices and Instrumentation
subject: Life Sciences
subject: photometry
subject: open-source
subject: pesticide
subject: affordable
subject: cholinesterase
subject: point-of-care test
subject: field-analysis

description: This project presents Open-Source Portable Photometric Platform. The Arduino Uno based photometer with programmable RGB LED as a light source. User can measure a colourful solutions and carry out enzymatic assays.
Due ore nello spazio con “Walking on the Moon”
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2019

Dal 23 settembre al 19 dicembre, a Milano, una mostra per celebrare il cinquantesimo anniversario dallo sbarco dell’uomo sulla Luna, organizzata dalla Bicocca in collaborazione con la Statale, il Politecnico e l’Istituto nazionale di astrofisica
Further evaluation of bootstrap resampling as a tool for radio-interferometric imaging fidelity assessment
Creators: name: Kemball, Athol
name: Martinsek, Adam
name: Mitra, Modhurita
name: Chiang, Hsin-Fang
Publisher: name: arXiv
Year: 2009
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We report on a broader evaluation of statistical bootstrap resampling methods as a tool for pixel-level calibration and imaging fidelity assessment in radio interferometry. Pixel-level imaging fidelity assessment is a challenging problem, important for the value it holds in robust scientific interpretation of interferometric images, enhancement of automated pipeline reduction systems needed to broaden the user community for these instruments, and understanding leadingedge direction-dependent calibration and imaging challenges for future telescopes such as the Square Kilometer Array. This new computational approach is now possible because of advances in statistical resampling for data with long-range dependence and the available performance of contemporary high-performance computing resources. We expand our earlier numerical evaluation to span a broader domain subset in simulated image fidelity and source brightness distribution morphologies. As before, we evaluate the statistical performance of the bootstrap resampling methods against direct Monte Carlo simulation. We find both model-based and subsample bootstrap methods to continue to show significant promise for the challenging problem of interferometric imaging fidelityassessment, when evaluated over the broader domain subset. We report on their measured statistical performance and guidelines for their use and application in practice. We also examine the performance of the underlying polarization self-calibration algorithm used in this study over a range of parallactic angle coverage.
description: 33 pages, 12 figures
Bromus sterilis
Creators: name: Cardona, Àngel Manuel Hernández
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Bromus
Bromus sterilis

description: Bromus sterilis L.
(bromus estèril). Natural d’Euràsia i nord d’Àfrica, i naturalitzat en altres parts de la Terra. Creix en herbassars, vores de camins i ermassos humits, en terrenys molt diversos. Apareix dispers per les zones altes i mitjanes.
description: Published as part of Cardona, Àngel Manuel Hernández, 2022, Catàleg actualitzat i claus d'identificació de les gramínies de Sant Llorenç del Munt i l'Obac (Barcelona), pp. 64-86 in Nemus 12 on page 69, DOI: 10.5281/zenodo.12170499
Assioni e progenitori di supernove
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2019

Quando esplodono, le supernova di tipo IIP brillano un po’ meno di quanto i calcoli degli astronomi prevederebbero. Dove e come avviene la perdita d’energia? Uno studio condotto da Oscar Straniero dell’Osservatorio astronomico Inaf d’Abruzzo, pubblicato lo scorso mese su The Astrophysical Journal, suggerisce un’ipotesi affascinante: i “responsabili” della perdita potrebbero essere particelle ancora ipotetiche – gli assioni
Chiral Odd Generalized Parton Distributions in Position Space
Creators: name: Mukherjee, A.
name: Chakrabarti, D.
name: Manohar, R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We report on a calculation of the chiral odd generalized parton distributions (GPDs) for non-zero skewness $ζ$ in transverse and longitudinal position spaces by taking Fourier transform with respect to the transverse and longitudinal momentum transfer respectively using overlaps of light-front wave functions (LFWFs).
description: Presented at the 18 th International Spin Physics Symposium, University of Virginia, Charlottesville, Virginia, USA, October 6-11, 2008
title: ÐÐ°ÑÑÐ±ÐµÐ¶Ð½Ð°Ñ ÐºÑÑ Ð½Ñ
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð´Ð»Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°ÑÐ° Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 19.03.04 Â«Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸ÑÂ»
titleType: Subtitle
Creators: name: Ð¡Ð¼Ð¾Ð»ÐµÐ½ÑÐµÐ²Ð°, Ð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: 2017
Subjects: ÐÐ¸ÑÐµÐ²ÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
ÐºÑÐ»Ð¸Ð½Ð°ÑÐ¸Ñ
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description: Ð£ÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 19.03.04 Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸ÑÂ». ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð½Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¸ÐºÐ° Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð¹ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ: ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ Ð¸Ð·ÑÑÐ°ÑÑ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¸ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÐ¹ Ð¾Ð¿ÑÑ Ð¿Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ; Ð³Ð¾ÑÐ¾Ð²Ð½Ð¾ÑÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¸ ÑÑÐ»ÑÐ³ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ ÐºÑÐ»ÑÑÑÑÐ½ÑÐ¼Ð¸ ÑÑÐ°Ð´Ð¸ÑÐ¸ÑÐ¼Ð¸ Ð¸ Ð¾Ð±ÑÑÐ°ÑÐ¼Ð¸ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ ÑÑÑÐ°Ð½ Ð¸ Ð½Ð°ÑÐ¾Ð´Ð¾Ð²; ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÑÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ Ð½Ð° ÐºÑÐ»Ð¸Ð½Ð°ÑÐ½ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð²ÐºÐ»ÑÑÐ°ÐµÑ ÑÐµÐ¼Ð°ÑÐ¸ÐºÑ, ÑÑÑÑÐºÑÑÑÑ, ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð´Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ. ÐÑÐ°Ð²Ð¸Ð»Ð° Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐ½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð·Ð°Ð¿Ð¸ÑÐºÐ¸ Ð¸ Ð¿Ð¾ÑÑÐ´Ð¾Ðº Ð·Ð°ÑÐ¸ÑÑ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÐÐ¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¡ÐÐ±ÐÐ£.
title: ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð·Ð°Ð½ÑÑÐ¸Ñ Ð¿Ð¾ Photoshop
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡ÐµÑÐ¸ÐºÐ¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
name: ÐÐ¾Ð´ÐºÐ¾Ð»ÑÐ·Ð¸Ð½Ð°, ÐÑÐ´Ð¼Ð¸Ð»Ð°
name: Ð¡ÐµÑÐ¸ÐºÐ¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
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: 2020
Subjects: 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
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