A magnetic reconnection model for explaining the multi-wavelength emission of the microquasars Cyg X-1 and Cyg X-3

Recent studies have indicated that cosmic ray acceleration by a first-order Fermi process in magnetic reconnection current sheets can be efficient enough in the surrounds of compact sources. In this work, we discuss this acceleration mechanism operating in the core region of galactic black hole bina...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2015-02
Hauptverfasser:	Khiali, Behrouz, Elisabete M de Gouveia Dal Pino, del Valle, Maria V
Format:	Artikel
Sprache:	eng
Schlagworte:	Acceleration Cosmic rays Current sheets Emission analysis High energy astronomy Microquasars Particle production Physics - High Energy Astrophysical Phenomena Spectral energy distribution Thermal emission
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!