Gamma-ray emission from binaries in context

Guillaume Dubus

doi:10.1016/j.crhy.2015.08.014

Gamma-ray emission from binaries in context
[Emission gamma des systèmes binaires]

Guillaume Dubus ^1,²

¹ Université Grenoble Alpes, IPAG, 38000 Grenoble, France
² CNRS, IPAG, 38000 Grenoble, France

Comptes Rendus. Physique, Volume 16 (2015) no. 6-7, pp. 661-673.

Résumé
Abstract

Plus d'une douzaine de systèmes binaires sont maintenant identifiés comme des sources variables de rayonnement gamma de haute énergie ( $0.1 – 100 GeV$ ). Cinq systèmes binaires sont également des sources de rayonnement gamma de très haute énergie ( $⩾ 100 GeV$ ). Les processus menant à l'émission de ce rayonnement sont variés. On peut néanmoins diviser ces systèmes en quatre grandes classes : les binaires gamma, dont le moteur est la rotation d'un pulsar ; les microquasars, dont le moteur est l'accrétion sur un trou noir ou une étoile à neutrons ; les novae, dont l'énergie provient de la combustion nucléaire à la surface d'une naine blanche ; les binaires à collision de vents, qui dissipent l'énergie cinétique de vents d'étoiles massives. On soupçonnait depuis longtemps que certaines classes de systèmes binaires devaient être associées à de l'émission gamma (les microquasars) ; pour d'autres classes, la découverte d'émission gamma a été une surprise (les novae). Je propose ici une brève revue de nos connaissances sur l'émission gamma de haute et très haute énergie dans les systèmes binaires, avec le souci de souligner les liens avec d'autres objets astrophysiques dans lesquels des processus similaires sont à l'oeuvre (nébuleuses de pulsar, noyaux actifs de galaxie, restes de supernova).

More than a dozen binary systems are now established as sources of variable, high-energy (HE, $0.1 – 100 GeV$ ) gamma rays. Five are also established sources of very-high-energy (VHE, $⩾ 100 GeV$ ) gamma rays. The mechanisms behind gamma-ray emission in binaries are very diverse. My current understanding is that they divide up into four types of systems: gamma-ray binaries, powered by pulsar rotation; microquasars, powered by accretion onto a black hole or neutron star; novae, powered by thermonuclear runaway on a white dwarf; colliding wind binaries, powered by stellar winds from massive stars. Some of these types had long been suspected to emit gamma rays (microquasars), others have taken the community by surprise (novae). My purpose here is to provide a brief review of the current status of gamma-ray emission from binaries, in the context of related objects where similar mechanisms are at work (pulsar wind nebulae, active galactic nuclei, supernova remnants).

Publié le : 2015-08-01

DOI : 10.1016/j.crhy.2015.08.014

Keywords: Acceleration of particles, Radiation mechanisms: non-thermal, Binaries: general, Gamma-rays: stars
Mot clés : Accélération de particules, Mécanismes de rayonnement non thermiques, Étoiles binaires, Rayonnement gamma : étoiles

Affiliations des auteurs :

Guillaume Dubus ^{1, 2}

¹ Université Grenoble Alpes, IPAG, 38000 Grenoble, France
² CNRS, IPAG, 38000 Grenoble, France

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Guillaume Dubus. Gamma-ray emission from binaries in context. Comptes Rendus. Physique, Volume 16 (2015) no. 6-7, pp. 661-673. doi : 10.1016/j.crhy.2015.08.014. https://comptes-rendus.academie-sciences.fr/physique/articles/10.1016/j.crhy.2015.08.014/

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