Mass‐Loss Rate and He/H Abundance of the Erupting Component in the Small Magellanic Cloud System HD 5980-Reference-Cited by-同舟云学术

Mass‐Loss Rate and He/H Abundance of the Erupting Component in the Small Magellanic Cloud System HD 5980

Published:1998-06 Issue:2 Volume:499 Page:889-897
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Koenigsberger G.,Pena M,Schmutz W.,Ayala S.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/499/i=2/a=889/pdf

Reference65 articles.

1. Barba, R. & Niemela, V. S. 1994, IAU Symp. 163, Wolf-Rayet Stars: Binaries, Colliding Winds and Evolution, ed. K. A. van der Hucht & P. Williams (Dordrecht: Kluwer), 254

2. Sudden Luminous Blue Variable--Like Behavior of the Wolf-Rayet Binary System HD 5980 in the Small Magellanic Cloud

3. Barba, R. H., Niemela, V. S. & Morrell, N. I. 1997, in ASP Conf. Ser. 120, Luminous Blue Variables: Massive Stars in Transition, ed. A. Nota & H. Lamers (San Francisco: ASP), 238

4. Barba, R. H., etal 1996, in Rev. Mexicana Astron. Astrofis. Conf. Ser. 5, Workshop on Colliding Winds in Binary Stars, ed. V. Niemela & N. Morrell (Mexico: Inst. de Astronomia), 85

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