Lithium and its isotopic ratio ⁶Li/⁷Li in the atmospheres of sharp-lined roAp stars γ Equulei and HD 166473

The lithium lines at 6708 Å for two sharp-lined roAp stars γ Equ and HD 166473 and at 6103 Å for γ Equ were analyzed in high resolution spectra. Three spectral synthesis codes – STARSP, ZEEMAN2, and SYNTHM – were used. New lines of the rare-earth elements from the DREAM database and lines calculated...

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Опубліковано в: :Кинематика и физика небесных тел
Дата:2005
Автори: Shavrina, A., Polosukhina, N., Khan, S., Pavlenko, Ya., Khalack, V., Wade, G.A., Quine, t P., Mikhailitska, N., Yushchenko, A., Gopka, V., Kudryavtsev, D.
Формат: Стаття
Мова:Англійська
Опубліковано: Головна астрономічна обсерваторія НАН України 2005
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Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/79662
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Lithium and its isotopic ratio ⁶Li/⁷Li in the atmospheres of sharp-lined roAp stars γ Equulei and HD 166473 / A. Shavrina, N. Polosukhina, S. Khan, Ya. Pavlenko, V. Khalack, G.A. Wade, P. Quinet, N. Mikhailitska, A. Yushchenko, V. Gopka, D. Kudryavtsev // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 295-298. — Бібліогр.: 16 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Shavrina, A.
Polosukhina, N.
Khan, S.
Pavlenko, Ya.
Khalack, V.
Wade, G.A.
Quine, t P.
Mikhailitska, N.
Yushchenko, A.
Gopka, V.
Kudryavtsev, D.
author_facet Shavrina, A.
Polosukhina, N.
Khan, S.
Pavlenko, Ya.
Khalack, V.
Wade, G.A.
Quine, t P.
Mikhailitska, N.
Yushchenko, A.
Gopka, V.
Kudryavtsev, D.
citation_txt Lithium and its isotopic ratio ⁶Li/⁷Li in the atmospheres of sharp-lined roAp stars γ Equulei and HD 166473 / A. Shavrina, N. Polosukhina, S. Khan, Ya. Pavlenko, V. Khalack, G.A. Wade, P. Quinet, N. Mikhailitska, A. Yushchenko, V. Gopka, D. Kudryavtsev // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 295-298. — Бібліогр.: 16 назв. — англ.
collection DSpace DC
container_title Кинематика и физика небесных тел
description The lithium lines at 6708 Å for two sharp-lined roAp stars γ Equ and HD 166473 and at 6103 Å for γ Equ were analyzed in high resolution spectra. Three spectral synthesis codes – STARSP, ZEEMAN2, and SYNTHM – were used. New lines of the rare-earth elements from the DREAM database and lines calculated on the basis of the NIST energy levels were included. Magnetic splitting and other line broadening processes were taken into account. Enhanced abundances of lithium in the atmospheres of the stars and high estimates of ⁶Li/⁷Li ratio (0.2 ÷ 0.5) can be explained by the Galactic Cosmic Ray (GCR) production due to spallation reactions and the preservation of original ⁶Li and ⁷Li by strong magnetic fields.
first_indexed 2025-11-24T05:51:30Z
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last_indexed 2025-11-24T05:51:30Z
publishDate 2005
publisher Головна астрономічна обсерваторія НАН України
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spelling Shavrina, A.
Polosukhina, N.
Khan, S.
Pavlenko, Ya.
Khalack, V.
Wade, G.A.
Quine, t P.
Mikhailitska, N.
Yushchenko, A.
Gopka, V.
Kudryavtsev, D.
2015-04-03T17:55:56Z
2015-04-03T17:55:56Z
2005
Lithium and its isotopic ratio ⁶Li/⁷Li in the atmospheres of sharp-lined roAp stars γ Equulei and HD 166473 / A. Shavrina, N. Polosukhina, S. Khan, Ya. Pavlenko, V. Khalack, G.A. Wade, P. Quinet, N. Mikhailitska, A. Yushchenko, V. Gopka, D. Kudryavtsev // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 295-298. — Бібліогр.: 16 назв. — англ.
0233-7665
https://nasplib.isofts.kiev.ua/handle/123456789/79662
The lithium lines at 6708 Å for two sharp-lined roAp stars γ Equ and HD 166473 and at 6103 Å for γ Equ were analyzed in high resolution spectra. Three spectral synthesis codes – STARSP, ZEEMAN2, and SYNTHM – were used. New lines of the rare-earth elements from the DREAM database and lines calculated on the basis of the NIST energy levels were included. Magnetic splitting and other line broadening processes were taken into account. Enhanced abundances of lithium in the atmospheres of the stars and high estimates of ⁶Li/⁷Li ratio (0.2 ÷ 0.5) can be explained by the Galactic Cosmic Ray (GCR) production due to spallation reactions and the preservation of original ⁶Li and ⁷Li by strong magnetic fields.
The authors are grateful to Dr. P. North for the ESO spectra and Dr. J. Zverko for the remarks to the manuscript.
en
Головна астрономічна обсерваторія НАН України
Кинематика и физика небесных тел
MS3: Physics of Stars and Galaxies
Lithium and its isotopic ratio ⁶Li/⁷Li in the atmospheres of sharp-lined roAp stars γ Equulei and HD 166473
Article
published earlier
spellingShingle Lithium and its isotopic ratio ⁶Li/⁷Li in the atmospheres of sharp-lined roAp stars γ Equulei and HD 166473
Shavrina, A.
Polosukhina, N.
Khan, S.
Pavlenko, Ya.
Khalack, V.
Wade, G.A.
Quine, t P.
Mikhailitska, N.
Yushchenko, A.
Gopka, V.
Kudryavtsev, D.
MS3: Physics of Stars and Galaxies
title Lithium and its isotopic ratio ⁶Li/⁷Li in the atmospheres of sharp-lined roAp stars γ Equulei and HD 166473
title_full Lithium and its isotopic ratio ⁶Li/⁷Li in the atmospheres of sharp-lined roAp stars γ Equulei and HD 166473
title_fullStr Lithium and its isotopic ratio ⁶Li/⁷Li in the atmospheres of sharp-lined roAp stars γ Equulei and HD 166473
title_full_unstemmed Lithium and its isotopic ratio ⁶Li/⁷Li in the atmospheres of sharp-lined roAp stars γ Equulei and HD 166473
title_short Lithium and its isotopic ratio ⁶Li/⁷Li in the atmospheres of sharp-lined roAp stars γ Equulei and HD 166473
title_sort lithium and its isotopic ratio ⁶li/⁷li in the atmospheres of sharp-lined roap stars γ equulei and hd 166473
topic MS3: Physics of Stars and Galaxies
topic_facet MS3: Physics of Stars and Galaxies
url https://nasplib.isofts.kiev.ua/handle/123456789/79662
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