Stellar spectroscopy methods for study of supernova remnants

We present the method for study of the characteristics of the supernova remnants using their absorption properties. The background radiation sources are several stars with wide range of distances. Main task is accurate extraction of stellar spectra from observations. For Vela Jr. supernova remnant w...

Повний опис

Збережено в:
Бібліографічні деталі
Дата:2011
Автори: Pakhomov, Yu.V., Chugai, N.N., Iyudin, A.F.
Формат: Стаття
Мова:English
Опубліковано: Advances in astronomy and space physics 2011
Назва видання:Advances in Astronomy and Space Physics
Теми:
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/118943
Теги: Додати тег
Немає тегів, Будьте першим, хто поставить тег для цього запису!
Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Stellar spectroscopy methods for study of supernova remnants / Yu.V. Pakhomov, N.N. Chugai, A.F. Iyudin // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 15-18. — Бібліогр.: 7 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id irk-123456789-118943
record_format dspace
spelling irk-123456789-1189432017-06-02T03:03:58Z Stellar spectroscopy methods for study of supernova remnants Pakhomov, Yu.V. Chugai, N.N. Iyudin, A.F. Physics of Stars and Galaxies We present the method for study of the characteristics of the supernova remnants using their absorption properties. The background radiation sources are several stars with wide range of distances. Main task is accurate extraction of stellar spectra from observations. For Vela Jr. supernova remnant we found the absence of typical broad absorption in the spectral lines of Ca ii doublet. Using modeles of supernovae remnants and data on radiation in ⁴⁴Ti γ-ray line we estimated the age and the distance to Vela Jr. We showed that a hypernova may be a probable candidate for Vela Jr. protogenitor. 2011 Article Stellar spectroscopy methods for study of supernova remnants / Yu.V. Pakhomov, N.N. Chugai, A.F. Iyudin // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 15-18. — Бібліогр.: 7 назв. — англ. 987-966-439-367-3 http://dspace.nbuv.gov.ua/handle/123456789/118943 en Advances in Astronomy and Space Physics Advances in astronomy and space physics
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
topic Physics of Stars and Galaxies
Physics of Stars and Galaxies
spellingShingle Physics of Stars and Galaxies
Physics of Stars and Galaxies
Pakhomov, Yu.V.
Chugai, N.N.
Iyudin, A.F.
Stellar spectroscopy methods for study of supernova remnants
Advances in Astronomy and Space Physics
description We present the method for study of the characteristics of the supernova remnants using their absorption properties. The background radiation sources are several stars with wide range of distances. Main task is accurate extraction of stellar spectra from observations. For Vela Jr. supernova remnant we found the absence of typical broad absorption in the spectral lines of Ca ii doublet. Using modeles of supernovae remnants and data on radiation in ⁴⁴Ti γ-ray line we estimated the age and the distance to Vela Jr. We showed that a hypernova may be a probable candidate for Vela Jr. protogenitor.
format Article
author Pakhomov, Yu.V.
Chugai, N.N.
Iyudin, A.F.
author_facet Pakhomov, Yu.V.
Chugai, N.N.
Iyudin, A.F.
author_sort Pakhomov, Yu.V.
title Stellar spectroscopy methods for study of supernova remnants
title_short Stellar spectroscopy methods for study of supernova remnants
title_full Stellar spectroscopy methods for study of supernova remnants
title_fullStr Stellar spectroscopy methods for study of supernova remnants
title_full_unstemmed Stellar spectroscopy methods for study of supernova remnants
title_sort stellar spectroscopy methods for study of supernova remnants
publisher Advances in astronomy and space physics
publishDate 2011
topic_facet Physics of Stars and Galaxies
url http://dspace.nbuv.gov.ua/handle/123456789/118943
citation_txt Stellar spectroscopy methods for study of supernova remnants / Yu.V. Pakhomov, N.N. Chugai, A.F. Iyudin // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 15-18. — Бібліогр.: 7 назв. — англ.
series Advances in Astronomy and Space Physics
work_keys_str_mv AT pakhomovyuv stellarspectroscopymethodsforstudyofsupernovaremnants
AT chugainn stellarspectroscopymethodsforstudyofsupernovaremnants
AT iyudinaf stellarspectroscopymethodsforstudyofsupernovaremnants
first_indexed 2023-10-18T20:33:23Z
last_indexed 2023-10-18T20:33:23Z
_version_ 1796150509039517696