Another X-Ray Brightening of H 1743-322 = IGR J1746-3213

Details Another X-Ray Brightening of H 1743-322 = IGR J1746-3213 Another X-Ray Brightening of H 1743-322 = IGR J1746-3213

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..301....1s&link_type=abstract

The Astronomer's Telegram, #301

Astronomy and Astrophysics

Astronomy

10

Request For Observations, Binaries, Black Holes, Transients

Scientific paper

The black hole candidate X-ray transient H 1743-322 = IGR J1746-3213 = XTE J17464-3213, which went into outburst in March 2003 (ATEL#132,#133) and decayed below the RXTE PCA sensitivity limit sometime between Nov 2 and 2004 Feb 7, while it was too close to the sun, has brightened again. On Jul 3, the PCA scans of the galactic bulge detected it at a 2-10 keV intensity of 16(1) mCrab and on Jul 7, it had risen to 69(2) mCrab.

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