DY Persei, the coolest metal-poor R CrB carbon star-Reference-Cited by-同舟云学术

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DY Persei, the coolest metal-poor R CrB carbon star

Published:2009-03 Issue:3 Volume:53 Page:187-202
ISSN:1063-7729
Container-title:Astronomy Reports
language:en
Short-container-title:Astron. Rep.

Author:

Yakovina L. A.,Pugach A. F.,Pavlenko Ya. V.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1134/S1063772909030019.pdf

Reference37 articles.

1. C. Hoffmeister, Veroff. Sternw. Sonneberg 1, 1 (1947).

2. D. Cameron and J. I. Nassau, Astrophys. J. 124, 346 (1956).

3. A. Alksnis and Z. Jumike, Investig. Sun Red Stars (Riga), 33, 83 (1990).

4. A. Alksnis, Baltic Astron. 3, 410 (1994).

5. B. E. Zhilyaev, M. Ya. Orlov, A. F. Pugach et al., RCrB Stars (Naukova Dumka, Kiev, 1978) [in Russian].

Cited by 10 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. HdC and EHe stars through the prism of Gaia DR3;Astronomy & Astrophysics;2024-04

2. HdC and EHe stars through the prism of Gaia DR3;Astronomy & Astrophysics;2024-04

3. The Carbon Star DY Persei May Be a Cool R Coronae Borealis Variable;The Astrophysical Journal;2023-04-28

4. A spectral classification system for hydrogen-deficient carbon stars;Monthly Notices of the Royal Astronomical Society;2023-02-02

5. Are DY Persei Stars Cooler Cousins of R Coronae Borealis Stars?;The Astrophysical Journal;2018-02-21

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