Hard X-ray brightening of Ginga 1843+009 seen by INTEGRAL

Details Hard X-ray brightening of Ginga 1843+009 seen by INTEGRAL Hard X-ray brightening of Ginga 1843+009 seen by INTEGRAL

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..472....1l&link_type=abstract

The Astronomer's Telegram, #472

Astronomy and Astrophysics

Astronomy

3

X-Ray, Gamma Ray, Pulsars, Transients

Scientific paper

The transient X-ray pulsar, Ginga 1843+009, appears to be undergoing a hard X-ray outburst brighter than the one reported in May 2003 (ATEL #159). The source has been observed during ISWT observations of the Scutum Arm region with INTEGRAL and was first detected when the source was in the field of view of the ISGRI imager on 2005-04-23T11:05 with a 20-60 keV count rate of ~3 cps, corresponding to ~20 mCrab.

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