On the nature of the Be star HR 7409 (7 Vul)-Reference-Cited by-同舟云学术

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On the nature of the Be star HR 7409 (7 Vul)

Published:2011-03-08 Issue:4 Volume:413 Page:2760-2766
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Vennes S.,Kawka A.,Jonić S.,Pirković I.,Iliev L.,Kubát J.,Šlechta M.,Németh P.,Kraus M.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/413/4/2760/2877444/mnras0413-2760.pdf

Reference66 articles.

1. Be stars in binaries

2. Rotational Velocities of B Stars

3. Dark impact and galactic star formation: origin of the Gould belt

4. The ROSAT all-sky survey catalogue of optically bright OB-type stars

Cited by 4 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. The CHARA Array Interferometric Program on the Multiplicity of Classical Be Stars: New Detections and Orbits of Stripped Subdwarf Companions;The Astrophysical Journal;2024-02-01

2. Classifying Be Star Variability With TESS. I. The Southern Ecliptic;The Astronomical Journal;2022-04-21

3. A new study of the spectroscopic binary 7 Vul with a Be star primary;Astronomy & Astrophysics;2020-07

4. Hot Subluminous Stars;Publications of the Astronomical Society of the Pacific;2016-07-12

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