A Failed outburst of H1743-322

Astronomy and Astrophysics – Astronomy

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X-Ray Binary Stars, Black Holes, Brightness, Jets, X-Ray Binaries, Galactic Nuclei, Circumnuclear Matter, And Bulges, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Jets, Outflows, And Bipolar Flows

Scientific paper

H1743-322 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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