Catalogue of particle-accelerating colliding-wind binaries

[en] Massive systems made of two or more stars are known to be the site for interesting physical processes -- including at least in some cases -- particle acceleration. Over the past decade, this topic motivated a particular effort to unveil the properties of these systems and characterize the circumstances responsible for the acceleration of particles and the potential role of pre-supernova massive stars in the production of high energy particles in our Galaxy. Although previous studies on this topic were mostly devoted to processes in general, or to a few individual objects in particular, a unified target-oriented census of particle-accelerating colliding-wind binaries (hereafter PACWBs) does not exist yet. This paper aims at making a general and unified census of these systems, emphasizing their main properties. A general discussion includes energetic considerations along with wind properties in relation with non-thermal emission processes that are likely at work in colliding-wind binaries. Finally, some guidelines for future observational and theoretical studies are drawn.

Disciplines :

Space science, astronomy & astrophysics

Author, co-author :

De Becker, Michaël ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO)

Raucq, Françoise ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Sciences spatiales

Language :

English

Title :

Catalogue of particle-accelerating colliding-wind binaries

Publication date :

30 September 2013

Journal title :

Astronomy and Astrophysics

ISSN :

0004-6361

eISSN :

1432-0746

Publisher :

EDP Sciences, Les Ulis, France

Volume :

558

Pages :

A28

Peer reviewed :

Peer Reviewed verified by ORBi

Additional URL :

http://www.aanda.org/articles/aa/full_html/2013/10/aa22074-13/aa22074-13.html

Available on ORBi :

since 15 August 2013

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133 (2 by ULiège)

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