H1743-322 X-ray Rise

Details H1743-322 X-ray Rise H1743-322 X-ray Rise

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..576....1s&link_type=abstract

The Astronomer's Telegram, #576

Astronomy and Astrophysics

Astronomy

3

X-Ray, Black Holes, Transients

Scientific paper

RXTE observations show that H1743-322 = IGR J1746-3213 = XTE J17464-3213 is again active in X-rays as well as radio (see Atel #575). The source was below the ASM 3-sigma day average sensitivity limit on Aug 5, but on Aug 6 the ASM saw a day average of 21(8)mCrab. A PCA scan on Aug 7, 13:20 UTC confirmed that the source was on, detecting 27.4(1.2) mCrab, 2-10 keV. On Aug 10, at 10:36 UTC, the PCA found that the source had risen to 57.0(1.8) mcrab.

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