Gamma rays from clumpy wind-jet interactions in high-mass microquasars

Context. The stellar winds of the massive stars in high-mass microquasars are thought to be inhomogeneous. The interaction of these inhomogeneities, or clumps, with the jets of these objects may be a major factor in gamma-ray production. Aims. Our goal is to characterize a typical scenario of clum...

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Detalles Bibliográficos
Autores principales:	Cita, V. M. de la, Palacio, Santiago del, Bosch Ramon, V., Paredes Fortuny, X., Romero, Gustavo Esteban, Khangulyan, D.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2017
Materias:	Ciencias Astronómicas Acceleration of particles Accretion, accretion disks Binaries: general Gamma rays: stars Stars: early-type X-rays: binaries
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/87683
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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