INVESTIGADORES
ROMERO Gustavo Esteban
artículos
Título:
Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
Autor/es:
BOSCH-RAMON, V.; PAREDES, J. M.; ROMERO, G. E.; TORRES, D. F.
Revista:
Chinese Journal of Astronomy and Astrophysics
Editorial:
Science Press
Referencias:
Lugar: Marrickville NSW; Año: 2005 vol. 5 p. 284 - 288
ISSN:
1009-9271
Resumen:
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.
