THE HD 5980 MULTIPLE SYSTEM: MASSES AND EVOLUTIONARY STATUS-Reference-Cited by-同舟云学术

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THE HD 5980 MULTIPLE SYSTEM: MASSES AND EVOLUTIONARY STATUS

Published:2014-09-03 Issue:4 Volume:148 Page:62
ISSN:1538-3881
Container-title:The Astronomical Journal
language:
Short-container-title:AJ

Author:

Koenigsberger Gloria,Morrell Nidia,Hillier D. John,Gamen Roberto,Schneider Fabian R. N.,González-Jiménez Nicolás,Langer Norbert,Barbá Rodolfo

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/1538-3881/148/i=4/a=62/pdf

Reference45 articles.

1. Wolf-Rayet stars in the Magellanic Clouds. II - The peculiar eclipsing binary HD 5980 in the SMC

2. Wolf-Rayet Stars and Interrelations with other Massive Stars in Galaxies

3. Rotating massive main-sequence stars

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1. An absence of binary companions to Wolf-Rayet stars in the Small Magellanic Cloud;Astronomy & Astrophysics;2024-09

2. Investigating the Chemically Homogeneous Evolution Channel and Its Role in the Formation of the Enigmatic Binary Black Hole Progenitor Candidate HD 5980;The Astrophysical Journal;2024-04-22

3. Binary stars in the new millennium;Progress in Particle and Nuclear Physics;2024-01

4. Constraints on the multiplicity of the most massive stars known: R136 a1, a2, a3, and c;Astronomy & Astrophysics;2023-11

5. X-Shooting ULLYSES: Massive stars at low metallicity;Astronomy & Astrophysics;2023-07

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