Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pasj...57..465y&link_type=abstract
Publications of the Astronomical Society of Japan, Vol.57, No.3, pp. 465-469
Astronomy and Astrophysics
Astronomy
1
Accretion: Accretion Disks, Stars: Binaries: Close, X-Rays: Spectra, X-Rays: Stars, X-Rays: Transients
Scientific paper
A new X-ray source was discovered in the Norma region with Ginga in 1988 April. The source position, derived from one-dimensional scan data, and its spectral properties are presented. The X-ray emission was dominant below ˜ 6 keV and not found in other observations. Thus, it is thought to be an ultrasoft transient X-ray source. The X-ray spectrum, constructed by a scan fit technique, was well represented by either blackbody, thermal bremsstrahlung, power-law, or multicolor disk models. Although all of the spectral models were acceptable from a statistical point of view, the ultrasoft nature of the spectrum and the transient behavior suggest that this source is a candidate source of black hole binaries.
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