Quantitative spectroscopy of extreme helium stars Model atmospheres and a non-LTE abundance analysis of BD+10°2179

Author:

Kupfer T.,Przybilla N.,Heber U.,Jeffery C. S.ORCID,Behara N. T.,Butler K.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 11 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Atomic structure, electron-impact excitation and collisional-radiative modelling for Ar II;Journal of Quantitative Spectroscopy and Radiative Transfer;2024-10

2. EC 19529−4430: SALT identifies the most carbon- and metal-poor extreme helium star;Monthly Notices of the Royal Astronomical Society;2024-04-08

3. The distribution, kinematics, and luminosities of extreme helium stars as probes of their origin and evolution;Monthly Notices of the Royal Astronomical Society;2023-10-26

4. Quantitative spectroscopy of B-type supergiants;Astronomy & Astrophysics;2022-12

5. HD 144941: the most extreme helium-strong star;Astronomy & Astrophysics;2021-10

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