Optical photometry and Halpha Spectroscopy of SWIFT J1910.2-0546/MAXI J1910-057

Bibcode
2012ATel.4347....1C
Casares, J.; Rodriguez-Gil, P.; Zurita, C.; Ignacio Gonzalez Martinez-Pais ; Corradi, R. L. M.; Cornelisse, R.; Charles, Phil A.
Referencia bibliográfica

The Astronomer's Telegram, #4347

Fecha de publicación:
8
2012
Número de autores
7
Número de autores del IAC
5
Número de citas
10
Número de citas referidas
9
Descripción
We report on optical photometry and spectroscopy of the black hole X-ray transient Swift J1910.2-0546/MAXI J1910-057 (Krimm at al. ATel #4139, Usui et al. ATel #4140). R-band photometry (time resolution 27s) over an interval of 3.1 hr was obtained using ALFOSC on the 2.5m Nordic Optical Telescope (NOT) on the night of 21 July 2012. The light curve is dominated by flickering superimposed on a smooth, approximately sinusoidal variability of amplitude ~0.02 mags and ~4 hr time scale.
Proyectos relacionados
Representación de la variable cataclísmica SS Cygni (Chris Moran)
Estrellas Binarias
El estudio de las estrellas binarias es una parte esencial de la astrofísica estelar. Una gran parte de las estrellas de nuestra Galaxia y de otras galaxias se ha formado en sistemas binarios o múltiples, por lo que entender la estructura y evolución de estos sistemas es importante desde el punto de vista estelar y galáctico. Un aspecto en el que
Pablo
Rodríguez Gil
En ejecución
Tipo
Sin árbitro
Física estelar e interestelar (FEEI)

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