Magnetised accretion discs in Kerr spacetimes

Context. Observational data from X-ray binary systems provide strong evidence of astronomical objects that are too massive and compact to be explained as neutron or hybrid stars. When these systems are in the thermal (high/soft) state, they emit mainly in the 0. 1-5 keV energy range. This emission c...

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Detalles Bibliográficos
Autores principales:	Ranea Sandoval, Ignacio Francisco, García, Federico
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2015
Materias:	Astronomía Accretion, accretion disks Black hole physics Gravitational lensing: Micro Line: Profiles Magnetic fields
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/86178
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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