SAX J1750.8-2900 is returning to quiescence

Details SAX J1750.8-2900 is returning to quiescence SAX J1750.8-2900 is returning to quiescence

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1662....1l&link_type=abstract

The Astronomer's Telegram, #1662

Astronomy and Astrophysics

Astronomy

3

X-Ray, Binaries, Neutron Stars, Transients

Scientific paper

The neutron star transient SAX J1750.8-2900 has been in outburst since March 15th, 2008 (ATel #1425). The X-ray flux started to decay around mid May and fell below the detection threshold of RXTE-ASM and Swift-BAT around August 2nd and 8th, respectively. We report here on a Swift-XRT observation of the source during its transition to the quiescent state. Swift observed the field on August 14th.

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