B and Be-stars in the young open stellar clusters NGC 659 and NGC 7419-Reference-Cited by-同舟云学术

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B and Be-stars in the young open stellar clusters NGC 659 and NGC 7419

Published:2011-03 Issue:1 Volume:54 Page:52-67
ISSN:0571-7256
Container-title:Astrophysics
language:en
Short-container-title:Astrophysics

Author:

Malchenko S. L.,Tarasov A. E.

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s10511-011-9157-x.pdf

Reference27 articles.

1. S. Kriz and P. Harmanec, Bull. Astron. Inst. Czechosl. 26 (2), 65 (1975).

2. P. Harmanec, in: M. A. Smith, H. F. Henrichs, and J. Fabregat, eds., IAU Coll. 175 (The Be Phenomenon in Early Type Stars), Publ. Astron. Soc. Pacif. Conf. Ser. 214, 13 (2000).

3. J. C. Mermilliod, Astron. Astrophys. 109, 48 (1982).

4. A. Slettebak, Astrophys. J. Suppl. Ser. 59, 769 (1985).

5. J. Fabregat and J. M. Torrejón, Astron. Astrophys. 375, 451 (2000).

Cited by 3 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. Hα Photometry of Be Stars in the Cluster NGC 7419;Research Notes of the AAS;2019-05-02

2. Be Stars in Open Stellar Clusters;Astrophysics;2017-06

3. NGC 7419 as a template for red supergiant clusters;Astronomy & Astrophysics;2013-04

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