An Ultrasoft Transient X-Ray Source in the Norma Region Discovered with Ginga
Abstract
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.
- Publication:
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Publications of the Astronomical Society of Japan
- Pub Date:
- June 2005
- DOI:
- Bibcode:
- 2005PASJ...57..465Y
- Keywords:
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- accretion: accretion disks;
- stars: binaries: close;
- X-rays: spectra;
- X-rays: stars;
- X-rays: transients