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Gabriela Montes, Ricardo F. González, Jorge Cantó, Miguel A. Pérez-Torres & Antonio Alberdi

Thermal Radio Emission from Radiative Shocks in Colliding Stellar Winds

(Volume 80 - Année 2011)
Article
Open Access

Abstract

We present a semi-analytic model for computing the thermal radio continuum emission from radiative shocks within colliding wind binaries. Assuming a thin shell approximation, we determine the contribution of the wind collision region (WCR) to the total thermal emission for close binaries. We investigate the effect of the binary separation and the stellar wind parameters on the total spectrum. In addition, we point out the relevance of taking into account this contribution for the correct interpretation of the observations, and the accuracy of the stellar wind parameters derived from them.

Pour citer cet article

Gabriela Montes, Ricardo F. González, Jorge Cantó, Miguel A. Pérez-Torres & Antonio Alberdi, «Thermal Radio Emission from Radiative Shocks in Colliding Stellar Winds», Bulletin de la Société Royale des Sciences de Liège [En ligne], Volume 80 - Année 2011, 704 - 708 URL : http://popups.ulg.be/0037-9565/index.php?id=3175.

A propos de : Gabriela Montes

Instituto de Astrofísica de Andalucía, IAA-CSIC, Granada, Spain

A propos de : Ricardo F. González

Centro de Radioastronomía y Astrofísica, CRyA-UNAM, Morelia, Mexico

A propos de : Jorge Cantó

Instituto de Astronomía, IA-UNAM, Mexico, D.F., Mexico

A propos de : Miguel A. Pérez-Torres

Instituto de Astrofísica de Andalucía, IAA-CSIC, Granada, Spain

A propos de : Antonio Alberdi

Instituto de Astrofísica de Andalucía, IAA-CSIC, Granada, Spain