Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-25T18:44:34.404Z Has data issue: false hasContentIssue false
  • English
  • Français

Is there a Connection Between Non-Synchronous Rotation and X-Ray Emission in Massive Binary Systems?

Published online by Cambridge University Press:  26 May 2016

Sinhué Haro ,
Juan Antonio Juárez  and
Gloria Koenigsberger
Sinhué Haro
Affiliation:
Instituto de Astronomía, UNAM, Mexico D.F. 04510
Juan Antonio Juárez
Affiliation:
Instituto de Astronomía, UNAM, Mexico D.F. 04510
Gloria Koenigsberger
Affiliation:
Centro de Ciencias Físicas, UNAM, Cuernavaca, Morelos, 62251

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.

A correlation between orbital period and log(LX/Lbol) is found for a sample of B-type binary systems. We suggest that wind-wind collisions are the likely mechanism for generating the X-ray emission, and that the mass-loss rates may be enhanced in non-synchronously rotating systems due to the oscillations that are excited by the tidal forces.

Type
Session 1 Observations of Rotating Stars
Information
Symposium - International Astronomical Union , Volume 215: Stellar Rotation , 2004 , pp. 163 - 165
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

, Abt, , Levato, , Grosso 2002, ApJ 573, 359.Google Scholar
Batten, A.H., Fletcher, J.M., & MacCarthy, D.G. 1989, Eighth Catalogue of the Orbital Elements of Spectroscopic Binary Systems (Publ. Dom Astrophys. Obs. Victoria 17; Victoria:DOA).Google Scholar
Berghoefer, T.W., Schmitt, J.H.M.M., Cassinelli, J.P. 1996, A&AS 118, 481.Google Scholar
Moreno, E. & Koenigsberger, G. 1999, RMA&A 35, 157.Google Scholar
Koenigsberger, G., Moreno, E., & Cervantes, F., 2002, in IAU Symposium # 212, van der Hucht, Herrero & , Esteban (ed.), p. 101.CrossRefGoogle Scholar