{ "id": "astro-ph/0407450", "version": "v1", "published": "2004-07-21T15:03:47.000Z", "updated": "2004-07-21T15:03:47.000Z", "title": "Gamma-Ray Emission From Be/X-Ray Binaries", "authors": [ "Mariana Orellana", "Gustavo E. Romero" ], "comment": "14 pages, to appear in: \"The multiwavelength approach to unidentified gamma-ray sources\", Eds. K. S. Cheng & G.E. Romero, Kluwer Academic Publisher (Astrophysics and Space Sciences Journal). The present version has two additional figures respect to the version to be published in the journal", "journal": "Astrophys.Space Sci. 297 (2005) 167-178", "doi": "10.1007/s10509-005-7618-6", "categories": [ "astro-ph" ], "abstract": "Be/X-ray binaries are systems formed by a massive Be star and a magnetized neutron star, usually in an eccentric orbit. The Be star has strong equatorial winds occasionally forming a circumstellar disk. When the neutron star intersects the disk the accretion rate dramatically increases and a transient accretion disk can be formed around the compact object. This disk can last longer than a single orbit in the case of major outbursts. If the disk rotates faster than the neutron star, the Cheng-Ruderman mechanism can produce a current of relativistic protons that would impact onto the disk surface, producing gamma-rays from neutral pion decays and initiating electromagnetic cascades inside the disk. In this paper we present calculations of the evolution of the disk parameters during both major and minor X-ray events, and we discuss the generation of gamma-ray emission at different energies within a variety of models that include both screened and unscreened disks.", "revisions": [ { "version": "v1", "updated": "2004-07-21T15:03:47.000Z" } ], "analyses": { "keywords": [ "gamma-ray emission", "be/x-ray binaries", "equatorial winds occasionally forming", "disk rotates faster", "minor x-ray events" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 14, "language": "en", "license": "arXiv", "status": "editable", "inspire": 654895 } } }