Mass—luminosity relation and pulsational properties of Wolf—Rayet stars-Reference-Cited by-同舟云学术

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Mass—luminosity relation and pulsational properties of Wolf—Rayet stars

Published:2008-11 Issue:11 Volume:34 Page:772-784
ISSN:1063-7737
Container-title:Astronomy Letters
language:en
Short-container-title:Astron. Lett.

Author:

Fadeyev Yu. A.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1134/S1063773708110066.pdf

Reference21 articles.

1. M. Beech and R. Mitalas, Astron. Astrophys. 262, 483 (1992).

2. E. A. Dorfi, A. Gautschy, and H. Saio, Astron. Astrophys. 453, L35 (2006).

3. C. Doom, J. P. de Greve, and C. de Loore, Astrophys. J. 303, 136 (1986).

4. Yu. A. Fadeyev, Pis’ma Astron. Zh. 33, 775 (2007) [Astron. Lett. 33, 692 (2007)].

5. Yu. A. Fadeyev, Astron. Zh. 85, 716 (2008) [Astron. Rep. 52, 645 (2008)].

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1. Spectroscopic Observations of Ten Galactic Wolf–Rayet Stars at Bosscha Observatory: Determination of Stellar Parameters and Mass-loss Rates;Research in Astronomy and Astrophysics;2024-08-22

2. References;Pulsating Stars;2015-08-21

3. The photometric variability of the WC9-type Wolf-Rayet star WR 103;Astrophysics and Space Science;2013-02-07

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5. Radial pulsations of massive main-sequence stars;Astronomy Letters;2011-01

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