XTE J1811-197: Position and Fluxes of A New 5.54 s pulsar

Details XTE J1811-197: Position and Fluxes of A New 5.54 s pulsar XTE J1811-197: Position and Fluxes of A New 5.54 s pulsar

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003atel..167....1m&link_type=abstract

The Astronomer's Telegram, #167

Astronomy and Astrophysics

Astronomy

3

X-Ray, Request For Observations, Neutron Stars, Pulsars, Soft Gamma-Ray Repeaters, Transients

Scientific paper

In Ibrahim et al. (GCN #2306), we reported the presence of a 5.54 s pulsar, detected in the RXTE PCA field of an observation of SGR 1806-20. At the time, we speculated that the pulsar could either be the source of soft gamma repeater bursts seen by the IPN (GCN #2297); or, a previously unknown pulsar simultaneously active with the known SGR 1806-20. Since then, Hurley et al. (GCN #2308) have concluded that HETE data agree with the IPN that SGR 1806-20 is the likely source of the bursts.

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