H 1743-322 approaching state transition

Astronomy and Astrophysics – Astronomy

Scientific paper

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X-Ray, Binaries, Black Holes, Transients

Scientific paper

After the four RXTE observations reported in ATel #2788, the spectrum of the black-hole binary H 1743-322 softened progressively, while at the same time the characteristic frequencies of its fast time variability increased. This indicated that the system had entered the hard intermediate state and was probably heading to a state transition to the soft intermediate state. This transition is usually associated to (although not coincident with) the ejection of relativistic jets.

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