1E 1207.4-5209: The Isolated X-ray Pulsar in the PKS 1209--51/52 Supernova Remnant

Details 1E 1207.4-5209: The Isolated X-ray Pulsar in the PKS 1209--51/52 Supernova Remnant 1E 1207.4-5209: The Isolated X-ray Pulsar in the PKS 1209--51/52 Supernova Remnant

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..aprk11006s&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

The central source of the supernova remnant PKS 1209--51/52 was observed with the Advanced CCD Imaging Spectrometer aboard Chandra X-ray observatory on 2000 January 6-7 in the Continuous Clocking mode. The discovery of a period, P=0.42412927 seconds, reported by Zavlin et al. (2000), shows that the source is a neutron star. This source was re-observed with Chandra on 2002 January 5-6 in the same mode. We will present the results of this observation and discuss the implication of the measured period derivative and the observed spectrum of this source.

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