Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500

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, concentrate...

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Detalles Bibliográficos
Autores principales: Bosch Ramon, Valentí, Paredes, J. M., Romero, Gustavo Esteban, Torres, Diego F.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2005
Materias:
Ciencias Astronómicas
X-rays: binaries
Stars: winds, outflows
gamma-rays: observations
gamma-rays: theory
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/127087
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-127087
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
X-rays: binaries
Stars: winds, outflows
gamma-rays: observations
gamma-rays: theory
spellingShingle Ciencias Astronómicas
X-rays: binaries
Stars: winds, outflows
gamma-rays: observations
gamma-rays: theory
Bosch Ramon, Valentí
Paredes, J. M.
Romero, Gustavo Esteban
Torres, Diego F.
Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
topic_facet Ciencias Astronómicas
X-rays: binaries
Stars: winds, outflows
gamma-rays: observations
gamma-rays: theory
description 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.
format Articulo
Articulo
author Bosch Ramon, Valentí
Paredes, J. M.
Romero, Gustavo Esteban
Torres, Diego F.
author_facet Bosch Ramon, Valentí
Paredes, J. M.
Romero, Gustavo Esteban
Torres, Diego F.
author_sort Bosch Ramon, Valentí
title Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
title_short Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
title_full Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
title_fullStr Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
title_full_unstemmed Microquasar Models for 3EG J1828+0142 and 3EG J1735-1500
title_sort microquasar models for 3eg j1828+0142 and 3eg j1735-1500
publishDate 2005
url http://sedici.unlp.edu.ar/handle/10915/127087
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AT romerogustavoesteban microquasarmodelsfor3egj18280142and3egj17351500
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