Observations of GX 339-4 in 1996

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dc.creatorSmith, I. A.
dc.creatorLiang, E. P.
dc.creatorLin, D.
dc.creatorBottcher, M.
dc.creatorMoss, M.
dc.creatorCrider, A.
dc.creatorFilippenko, A. V.
dc.creatorLeonard, D. C.
dc.creatorFender, R. P.
dc.creatorDurouchoux, Ph.
dc.creatorCorbel, S.
dc.creatorSood, R.
dc.date1998-12-08
dc.date.accessioned2026-07-07T02:29:33Z
dc.date.available2026-07-07T02:29:33Z
dc.descriptionGX 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.
dc.descriptionTo appear in Astrophysical Letters and Communications: 3rd INTEGRAL Workshop proceedings. 4 pages. 0 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9812163
dc.identifierhttp://arxiv.org/abs/astro-ph/9812163
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13515
dc.subjectAstrophysics
dc.titleObservations of GX 339-4 in 1996
dc.typetext

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