Identification of the optical and near-infrared counterpart of GRS 1758-258

Context. Understood to be a microquasar in the Galactic center region, GRS 1758-258 has not yet been unambiguously identified to have an optical/near-infrared counterpart, mainly because of the high absorption and the historic lack of suitable astrometric stars, which led to the use of secondary ast...

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Detalles Bibliográficos
Autores principales: Muñoz-Arjonilla, A.J., Martí, J., Luque-Escamilla, P.L., Sánchez-Sutil, J.R., Sánchez-Ayaso, E., Combi, J.A., Mirabel, I.F.
Formato: JOUR
Materias:
Infrared: general
Radio continuum: stars
X-rays: binaries
X-rays: stars
1E 1740.7-2942
Archival image
Emission lines
Extragalactic origin
Galactic Center region
Infrared source
Low signal-to-noise ratio
Near Infrared
Near-infrared wavelength
Radio data
Spectral observations
X rays: stars
X-rays: Binaries
Infrared devices
Light sources
Signal to noise ratio
X rays
Stars
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v519_n1_p_MunozArjonilla
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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