RXTE and Swift observations of XTE J1751-305 Show a Return to Quiescence

Details RXTE and Swift observations of XTE J1751-305 Show a Return to Quiescence RXTE and Swift observations of XTE J1751-305 Show a Return to Quiescence

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1051....1m&link_type=abstract

The Astronomer's Telegram, #1051

Other

7

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

Scientific paper

The X-ray millisecond pulsar XTE J1751-305 was reported active on 04 April 2007 by RXTE (Markwardt & Swank, ATEL #1045) and INTEGRAL (Falanga et al., ATEL #1046). Follow-up observations were obtained by RXTE and Swift, which show the source is already returning to quiescence. The Swift observation began on 05 April 2007 16:25 UT and had a duration of about 2000 sec. The Swift XRT observation confirms the presence of XTE J1751-305, and no other bright source in the field of view.

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