XTE J1829-098: a New 7.8 s Period Pulsar

Details XTE J1829-098: a New 7.8 s Period Pulsar XTE J1829-098: a New 7.8 s Period Pulsar

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..317....1m&link_type=abstract

The Astronomer's Telegram, #317

Astronomy and Astrophysics

Astronomy

4

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

Scientific paper

Within the past three months, RXTE PCA monitoring observations of the galactic center region have been enlarged to include portions of the galactic plane on either side of the galactic bulge. The scans extend to about +/- 25 degrees in galactic longitude and +/- 4 degrees in galactic latitude. Scans on July 30.9 (UTC) detected a new source with intensity ~7 mCrab. In follow-up pointed PCA observations on August 5.3, the source was detected as an X-ray pulsar.

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