The LMXRB GX354-0 is flaring in the hard X-rays

Details The LMXRB GX354-0 is flaring in the hard X-rays The LMXRB GX354-0 is flaring in the hard X-rays

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..248....1z&link_type=abstract

The Astronomer's Telegram, #248

Astronomy and Astrophysics

Astronomy

12

X-Ray, Gamma Ray, Binaries, Neutron Stars, Transients

Scientific paper

GX 354-0 (also known as 4U 1728-34) has been monitored by INTEGRAL as part of the Galactic Center Deep Exposure almost continuously from 2004-02-16 until now. Over that period the source flux measured by IBIS/ISGRI between 20-60 keV featured a smooth increase with a maximum flux of 0.2 Crab measured on February 24th. The source flux then decreased by a factor of 5 on a time scale of one week. Below 10 keV the flux measured by JEM-X increased by a factor larger than 6 continuously on a timescale of 3 weeks.

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