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The IR counterpart of the black-hole candidate 4U 1630-47
release_xtwuyls74rd23plnvxbiux2p64
by
T. Augusteijn, M.H. van
Kerkwijk
Released
as a article
.
2001
Abstract
We present K band photometry of the region including the radio error box of
the soft X-ray transient 4U 1630-47 during its 1998 outburst. We detect a
variable source at K=16.1 mag located inside the radio error circle which we
identify as the counterpart to the X-ray source. We discuss the properties of
the source, and conclude that it is most likely a black-hole X-ray binary
similar to 4U 1543-47, GRO J1655-40 or SAX J1819.3-2525, containing a
relatively early-type secondary.
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astro-ph/0107337v1
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