Modeling of the spectrum of Cygnus OB2 No. 7 supergiant-Reference-Cited by-同舟云学术

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Modeling of the spectrum of Cygnus OB2 No. 7 supergiant

Published:2013-01 Issue:1 Volume:68 Page:87-100
ISSN:1990-3413
Container-title:Astrophysical Bulletin
language:en
Short-container-title:Astrophys. Bull.

Author:

Maryeva O. V.,Klochkova V. G.,Chentsov E. L.

Publisher

Pleiades Publishing Ltd

Subject

Astronomy and Astrophysics,Instrumentation

Link

http://link.springer.com/content/pdf/10.1134/S1990341313010082.pdf

Reference56 articles.

1. M. J. Seaton, Journal of Physics B-Atomic and Molecular Physics 20, 6363 (1987).

2. D. G. Hummer, K. A. Berrington, W. Eissner, et al., Astronom. and Astrophys. 279, 298 (1993).

3. S. N. Nahar, ASP Conf. Ser. 288, 651 (2003).

4. A. K. Pradhan, H. L. Zhang, S. N. Nahar, et al., Bull. of the American Astronom. Soc. 28, 1367 (1996).

5. C. A. Iglesias and F. J. Rogers, Astrophys. J. 371, 408 (1991).

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1. e-MERLIN 21 cm constraints on the mass-loss rates of OB stars in Cyg OB2;Monthly Notices of the Royal Astronomical Society;2016-08-02

2. Properties of Dwarf Stars in Cygnus OB2;Publications of the Astronomical Society of Australia;2016

3. Investigation of the brightest stars in the Cyg OB2 association;Proceedings of the International Astronomical Union;2014-06

4. Investigation of Cyg OB2 #11(O5 Ifc) by Modelling its Atmosphere;Publications of the Astronomical Society of Australia;2014

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