Smooth time variation spectra as a tool to study line profile variability in spectra of hot stars

Line profiles in spectra of almost all OB stars are variable. In many cases the line profile variations are extremely weak (not more than 1% of the continuum level). For detection of such micro line profile variations of various nature we used a smooth Time Variation Spectra method (smTVS). This met...

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Видавець:Головна астрономічна обсерваторія НАН України
Дата:2012
Автор: Sudnik, N.P.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2012
Назва видання:Advances in Astronomy and Space Physics
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/119105
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Цитувати:Smooth time variation spectra as a tool to study line profile variability in spectra of hot stars / N.P. Sudnik // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 5-8. — Бібліогр.: 10 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id irk-123456789-119105
record_format dspace
spelling irk-123456789-1191052017-06-05T03:03:59Z Smooth time variation spectra as a tool to study line profile variability in spectra of hot stars Sudnik, N.P. Line profiles in spectra of almost all OB stars are variable. In many cases the line profile variations are extremely weak (not more than 1% of the continuum level). For detection of such micro line profile variations of various nature we used a smooth Time Variation Spectra method (smTVS). This method appeared to be very sensitive and can be used to detect ultra weak line profile variations which can not be detected by other methods. We applied the smTVS method to detect the micro LPV in spectra of bright O stars λ Cep, λ Ori A and ζ Ori A. Spectra of these stars were obtained by using the 6-m and 1-m telescopes of the Northern Caucasus Special Astrophysical Observatory (Russia) and the 1.8-m telescope of Bohyunsan Astronomical Observatory (Korea). 2012 Article Smooth time variation spectra as a tool to study line profile variability in spectra of hot stars / N.P. Sudnik // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 5-8. — Бібліогр.: 10 назв. — англ. 2227-1481 http://dspace.nbuv.gov.ua/handle/123456789/119105 en Advances in Astronomy and Space Physics Головна астрономічна обсерваторія НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
description Line profiles in spectra of almost all OB stars are variable. In many cases the line profile variations are extremely weak (not more than 1% of the continuum level). For detection of such micro line profile variations of various nature we used a smooth Time Variation Spectra method (smTVS). This method appeared to be very sensitive and can be used to detect ultra weak line profile variations which can not be detected by other methods. We applied the smTVS method to detect the micro LPV in spectra of bright O stars λ Cep, λ Ori A and ζ Ori A. Spectra of these stars were obtained by using the 6-m and 1-m telescopes of the Northern Caucasus Special Astrophysical Observatory (Russia) and the 1.8-m telescope of Bohyunsan Astronomical Observatory (Korea).
format Article
author Sudnik, N.P.
spellingShingle Sudnik, N.P.
Smooth time variation spectra as a tool to study line profile variability in spectra of hot stars
Advances in Astronomy and Space Physics
author_facet Sudnik, N.P.
author_sort Sudnik, N.P.
title Smooth time variation spectra as a tool to study line profile variability in spectra of hot stars
title_short Smooth time variation spectra as a tool to study line profile variability in spectra of hot stars
title_full Smooth time variation spectra as a tool to study line profile variability in spectra of hot stars
title_fullStr Smooth time variation spectra as a tool to study line profile variability in spectra of hot stars
title_full_unstemmed Smooth time variation spectra as a tool to study line profile variability in spectra of hot stars
title_sort smooth time variation spectra as a tool to study line profile variability in spectra of hot stars
publisher Головна астрономічна обсерваторія НАН України
publishDate 2012
url http://dspace.nbuv.gov.ua/handle/123456789/119105
citation_txt Smooth time variation spectra as a tool to study line profile variability in spectra of hot stars / N.P. Sudnik // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 5-8. — Бібліогр.: 10 назв. — англ.
series Advances in Astronomy and Space Physics
work_keys_str_mv AT sudniknp smoothtimevariationspectraasatooltostudylineprofilevariabilityinspectraofhotstars
first_indexed 2023-10-18T20:33:48Z
last_indexed 2023-10-18T20:33:48Z
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