Observations of GX 339-4 in 1996

Details Observations of GX 339-4 in 1996 Observations of GX 339-4 in 1996

1998-12-08

arxiv.org/abs/astro-ph/9812163v1

Astronomy and Astrophysics

Astrophysics

To appear in Astrophysical Letters and Communications: 3rd INTEGRAL Workshop proceedings. 4 pages. 0 figures

Scientific paper

GX 339-4 is an unusual black hole candidate in that it is a persistent
source, being detected by X-ray telescopes most of the time, but it also has
nova-like flaring states. In 1996 we performed radio, optical, X-ray, and
gamma-ray observations of GX 339-4 when it was in a hard state (= soft X-ray
low state). Here we present a brief summary of some of the results.

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