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Si us plau utilitzeu sempre aquest identificador per citar o enllaçar aquest document: https://hdl.handle.net/2445/46863
Chorros relativistas de origen estelar: los microcuasares
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Galactic microquasars are certainly one of the most recent additions to the field of high energy Astrophysics. These new objects are just X-ray binaries with the ability to generate relativistic jets and their interest has been growing during the last decade. Today, they represent primary targets for all space based observatories working in the X-ray and [gamma]-ray domains. Behind such interest, there is hope that their study will assist us to understand some of the analog phenomena observed in distant quasars and active galactic nuclei, wich share with microquasars practically the same scaled-up physics. Microquasars are also believed to be among the different kind of sources responsible for the violent and ever changing appearance of the [gamma]-ray ski. In this paper we review the general situation of the microquasar topic, their identification and study, including comments on the recent observational and theoretical discoveries most relevant in our opinion.
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PAREDES I POY, Josep maria, MARTÍ RIBAS, Josep. Chorros relativistas de origen estelar: los microcuasares. _Boletín de la Sociedad Española de Astronomía _. 2002. Vol. 8, núm. 22-35. [consulta: 30 de gener de 2026]. [Disponible a: https://hdl.handle.net/2445/46863]