Cyclotron Line in XTE J0658-073

Details Cyclotron Line in XTE J0658-073 Cyclotron Line in XTE J0658-073

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003atel..200....1h&link_type=abstract

The Astronomer's Telegram, #200

Astronomy and Astrophysics

Astronomy

5

X-Ray, Neutron Stars, Pulsars, Transients

Scientific paper

Joint RXTE PCA and HEXTE spectral analysis of the 2003 October 20 observation of the 160.7 second accreting pulsar XTE J0658-073 (Morgan et al. 2003, ATEL #199) reveals a strong cyclotron line at ~35keV. We fit a range of continuum models typical of accreting pulsars to the pulse phase averaged spectra. In all cases, significant residual deviations characteristic of a cyclotron feature were detected above ~20keV.

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