A Failed Outburst Of H1743-322

X-RAY ASTRONOMY-2009: PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES, PROCEEDINGS(2010)

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摘要
H 1743-322 is a bright BHC observed by HEAO-1 in 1977. The source underwent again in outburst in 2003 after about 25 years. After the 2003 outburst (the brightest one) the source exhibited other 5 outbursts. We report a brief summary of the results found during a campaign of X-ray observations performed with RXTE during the two 2008 outbursts. In particular the October 2008 outburst showed a singular behaviour that has been rarely observed in transient X-ray binaries.
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关键词
X-ray Binaries,Galactic Black Holes
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