Optical and Infrared Light Curves of the Black-hole Binary GX 339-4

Details Optical and Infrared Light Curves of the Black-hole Binary GX 339-4 Optical and Infrared Light Curves of the Black-hole Binary GX 339-4

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.2010b&link_type=abstract

American Astronomical Society Meeting 210, #20.10; Bulletin of the American Astronomical Society, Vol. 39, p.123

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We present our light curves of the black-hole X-ray binary GX 339-4 in V-, I-, J-, and H-bands from 2002 to the present. There are several distinct and interesting features that are dependent on time and wavelength. We will indicate how these features may be related to emission from a non-thermal (possibly jets) or thermal (disk) source, or a combination of both. Data such as these are valuable in testing models of accretion disks and accretion processes.

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