Project VeSElkA: Vertical Stratification of Element Abundances in CP stars

A new research project on spectral analysis which aims to characterize the vertical stratification of element abundances in stellar atmospheres of chemically peculiar (CP) stars, is discussed in detail. Some results on detection of vertical abundance stratification in several slowly rotating main se...

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Збережено в:
Бібліографічні деталі
Опубліковано в: :Advances in Astronomy and Space Physics
Дата:2015
Автори: Khalack, V.R., LeBlanc, F.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2015
Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/119817
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Project VeSElkA: Vertical Stratification of Element Abundances in CP stars / V.R. Khalack, F. LeBlanc // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 1. — С. 3-10. — Бібліогр.: 61 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-119817
record_format dspace
spelling Khalack, V.R.
LeBlanc, F.
2017-06-09T20:28:02Z
2017-06-09T20:28:02Z
2015
Project VeSElkA: Vertical Stratification of Element Abundances in CP stars / V.R. Khalack, F. LeBlanc // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 1. — С. 3-10. — Бібліогр.: 61 назв. — англ.
2227-1481
DOI: 10.17721/2227-1481.5.3-10
https://nasplib.isofts.kiev.ua/handle/123456789/119817
A new research project on spectral analysis which aims to characterize the vertical stratification of element abundances in stellar atmospheres of chemically peculiar (CP) stars, is discussed in detail. Some results on detection of vertical abundance stratification in several slowly rotating main sequence CP stars are presented and considered as an indicator of the effectiveness of the atomic diffusion mechanism responsible for the observed peculiarities of chemical abundances. This study is carried out in the frame of Project VeSElkA (Vertical Stratification of Elements Abundance) for which 34 slowly rotating CP stars have been observed with the ESPaDOnS spectropolarimetre at CFHT.
We are thankful to the Faculté des Études Supérieures et de la Recherche de l'Université de Moncton and NSERC for research grants. The grids of stellar atmosphere models and corresponding fluxes have been generated using the supercomputer briarree of l'Université de Montréal, that operates under the guidance of Calcul Québec and Calcul Canada. The use of this supercomputer is funded by the Canadian Foundation for Innovation (CFI), NanoQuébec, RMGA and Research Fund of Québec - Nature and Technology (FRQNT). This paper has been typeset from a TEX/LATEX file prepared by the authors.
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
Project VeSElkA: Vertical Stratification of Element Abundances in CP stars
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Project VeSElkA: Vertical Stratification of Element Abundances in CP stars
spellingShingle Project VeSElkA: Vertical Stratification of Element Abundances in CP stars
Khalack, V.R.
LeBlanc, F.
title_short Project VeSElkA: Vertical Stratification of Element Abundances in CP stars
title_full Project VeSElkA: Vertical Stratification of Element Abundances in CP stars
title_fullStr Project VeSElkA: Vertical Stratification of Element Abundances in CP stars
title_full_unstemmed Project VeSElkA: Vertical Stratification of Element Abundances in CP stars
title_sort project veselka: vertical stratification of element abundances in cp stars
author Khalack, V.R.
LeBlanc, F.
author_facet Khalack, V.R.
LeBlanc, F.
publishDate 2015
language English
container_title Advances in Astronomy and Space Physics
publisher Головна астрономічна обсерваторія НАН України
format Article
description A new research project on spectral analysis which aims to characterize the vertical stratification of element abundances in stellar atmospheres of chemically peculiar (CP) stars, is discussed in detail. Some results on detection of vertical abundance stratification in several slowly rotating main sequence CP stars are presented and considered as an indicator of the effectiveness of the atomic diffusion mechanism responsible for the observed peculiarities of chemical abundances. This study is carried out in the frame of Project VeSElkA (Vertical Stratification of Elements Abundance) for which 34 slowly rotating CP stars have been observed with the ESPaDOnS spectropolarimetre at CFHT.
issn 2227-1481
url https://nasplib.isofts.kiev.ua/handle/123456789/119817
citation_txt Project VeSElkA: Vertical Stratification of Element Abundances in CP stars / V.R. Khalack, F. LeBlanc // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 1. — С. 3-10. — Бібліогр.: 61 назв. — англ.
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last_indexed 2025-11-28T12:05:43Z
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