The accreting millisecond pulsar HETE J1900.1-2455 is returning to quiescence

Details The accreting millisecond pulsar HETE J1900.1-2455 is returning to quiescence The accreting millisecond pulsar HETE J1900.1-2455 is returning to quiescence

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1086....1g&link_type=abstract

The Astronomer's Telegram, #1086

Astronomy and Astrophysics

Astronomy

4

X-Ray, Request For Observations, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

We report ongoing Rossi X-ray Timing Explorer (RXTE) monitoring observations of the accretion-powered millisecond pulsar HETE J1900.1-2455 (Kaaret et al. 2006, ApJ 638, 963). This source has been X-ray active continuously since it first went into outburst in June 2005 (see e.g. ATel #657), although the 377.3 Hz pulsations became undetectable in August 2005 and have not been detected since. The last two RXTE observations have found HETE J1900.1-2455 at the faintest flux level yet seen.

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