Observations of GX 339-4 in 1996
Astrophysics
2007-05-23 v1
Abstract
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.
Keywords
Cite
@article{arxiv.astro-ph/9812163,
title = {Observations of GX 339-4 in 1996},
author = {I. A. Smith and E. P. Liang and D. Lin and M. Bottcher and M. Moss and A. Crider and A. V. Filippenko and D. C. Leonard and R. P. Fender and Ph. Durouchoux and S. Corbel and R. Sood},
journal= {arXiv preprint arXiv:astro-ph/9812163},
year = {2007}
}
Comments
To appear in Astrophysical Letters and Communications: 3rd INTEGRAL Workshop proceedings. 4 pages. 0 figures