Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-23T02:24:30.904Z Has data issue: false hasContentIssue false
  • English
  • Français

Massive Close Binaries in the Magellanic Clouds

Published online by Cambridge University Press:  07 August 2017

Virpi S. Niemela  and
Lilia P. Bassino
Virpi S. Niemela
Affiliation:
1. Instituto de Astronomia y Fisica del Espacio, CC67, Suc. 28, 1428 Buenos Aires, Argentina
Lilia P. Bassino
Affiliation:
2. Facultad de Ciencias Astronomicas y Geofisicas, U.N.L.P., Paseo del Bosque s/n, 1900 La Plata, Argentina

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present spectroscopic orbits for 4 eclipsing binary systems in the Magellanic Clouds. The minimum masses that we find for the binary components in the LMC are: 34 + 17 M⊙ for HV 2241 and 26 + 15 M⊙ for HV 2543, and for the ones in the SMC: 21 + 25 M⊙ for AzV 73 and 17 + 19 M⊙ for HV 1620.

Type
Oral and Contributed Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 497 - 499
Copyright
Copyright © Kluwer 1992 

References

Davidge, T.J. (1987), Astron. J. 94, 1169.Google Scholar
Davidge, T.J. (1988), Astron. J. 95, 731.Google Scholar
Payne-Gaposchkin, C.H. and Gaposchkin, S. (1966), Smithson. Cont. Astrophys. No. 9.CrossRefGoogle Scholar
Payne-Gaposchkin, C.H. (1971), Smithson. Cont. Astrophys. No. 13.Google Scholar
Shapley, H. and McKibben Nail, V. (1953), Proceedings of the N.A.S. 39, 1.CrossRefGoogle Scholar