Observations of GX 339-4 in 1996
Smith, I. A. · Liang, E. P. · Lin, D. · Bottcher, M. · Moss, M. · Crider, A. · Filippenko, A. V. · Leonard, D. C. · Fender, R. P. · Durouchoux, Ph. · Corbel, S. · Sood, R.
Original · EN
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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