Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/45390
Title: Microquasar models for 3EG J1828+0142 and 3EG J1735-1500
Author: Bosch i Ramon, Valentí
Paredes i Poy, Josep Maria
Romero, Gustavo E.
Torres, Diego F.
Keywords: Estels binaris de raigs X
Estels
Vents
Raigs gamma
Astronomia de raigs gamma
Astrofísica
X-ray binaries
Stars
Winds
Gamma rays
Gamma ray astronomy
Astrophysics
Issue Date: 2005
Publisher: Chinese Academy of Sciences
Abstract: Microquasars are promising candidates to emit high-energy gamma-rays. Moreover, statistical studies show that variable EGRET sources at low galactic latitudes could be associated with the inner spiral arms. The variable nature and the location in the Galaxy of the high-mass microquasars, concentrated in the galactic plane and within 55 degrees from the galactic center, give to these objects the status of likely counterparts of the variable low-latitude EGRET sources. We consider in this work the two most variable EGRET sources at low-latitudes: 3EG J1828+0142 and 3EG J1735-1500, proposing a microquasar model to explain the EGRET data in consistency with the observations at lower energies (from radio frequencies to soft gamma-rays) within the EGRET error box.
Note: Versió postprint del document publicat a: http://dx.doi.org/10.1088/1009-9271/5/S1/284
It is part of: Chinese Journal of Astronomy and Astrophysics, 2005, vol. 5, p. 284-288
Related resource: http://dx.doi.org/10.1088/1009-9271/5/S1/284
URI: http://hdl.handle.net/2445/45390
ISSN: 1009-9271
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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