Continuing activity of the 2.65 ms accretion-powered pulsar HETE J1900.1-2455

Details Continuing activity of the 2.65 ms accretion-powered pulsar HETE J1900.1-2455 Continuing activity of the 2.65 ms accretion-powered pulsar HETE J1900.1-2455

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..657....1g&link_type=abstract

The Astronomer's Telegram, #657

Other

10

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

Scientific paper

We report on the ongoing monitoring of the 2.65 ms pulsar, HETE J1900.1-2455 (ATels 516, 523, 525, 526, 538 and others) with the Rossi X-ray Timing Explorer (RXTE). The source remains active at a flux of approximately 9e-10 ergs/cm2/s (2.5-25 keV), more than 150 d after the outburst commenced (around June 14). This is the longest outburst of any of the accretion-powered millisecond pulsars, by a factor of approximately three.

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