Properties and nature of Be stars-Reference-Cited by-同舟云学术

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Properties and nature of Be stars

Published:2006-08-16 Issue:3 Volume:455 Page:1037-1052
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Linnell A. P.,Harmanec P.,Koubský P.,Božić H.,Yang S.,Ruždjak D.,Sudar D.,Libich J.,Eenens P.,Krpata J.,Wolf M.,Škoda P.,Šlechta M.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20053792/pdf

Reference54 articles.

1. Becker, W. in Basic Astronomical Data, Stars and Stellar Systems Vol. III, (Chicago: Univ. of Chicago Press) ed. K. A. Strand, 241

2. 14 Lacertae: A case of shell–orbit coupling?

3. The evolution of the theoretical bolometric albedo in close binary systems

4. Cox, A. N. 2000, Allen's Astrophysical Quantities (New York: Springer)

5. A Statistical Study of Threshold Rotation Rates for the Formation of Disks around Be Stars

Cited by 12 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. V1294 Aql = HD 184279: A bad boy among Be stars or an important clue to the Be phenomenon?;Astronomy & Astrophysics;2022-10

2. Investigating the lack of main-sequence companions to massive Be stars;Astronomy & Astrophysics;2020-09

3. Close Binary Perspectives;Galaxies;2020-08-03

4. An analytic self-gravitating disk model: inferences and logical structure;Contributions of the Astronomical Observatory Skalnaté Pleso;2020-03-01

5. Self-gravitating Semi-transparent Circumstellar Disks: An Analytic Model;The Astrophysical Journal;2018-12-06

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