MAXI/GSC detects a re-brightening from the black hole candidate H 1743-322

Details MAXI/GSC detects a re-brightening from the black hole candidate H 1743-322 MAXI/GSC detects a re-brightening from the black hole candidate H 1743-322

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2774....1n&link_type=abstract

The Astronomer's Telegram, #2774

Astronomy and Astrophysics

Astronomy

1

X-Ray, Binaries, Black Holes

Scientific paper

An increase of X-ray flux of the black hole candidate H 1743-322 was observed with MAXI/GSC on 2010 August 5 at 53+-5 mCrab in the 2-20 keV range. The RXTE/PCA Galactic scan observations and the Swift BAT hard X-ray monitor also show a rapid increase in both soft and hard X-rays. This indicates a beginning of a new outburst where the source would be in the low/hard state. Multi-wavelength observations of this initial stage of the outburst are strongly encouraged.

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