Observations of SGRs and AXPs with ASCA

Details Observations of SGRs and AXPs with ASCA Observations of SGRs and AXPs with ASCA

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...197.1702m&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #17.02; Bulletin of the American Astronomical Society, Vol. 32, p.1432

Astronomy and Astrophysics

Astronomy

Scientific paper

Anomalous x-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs) are x-ray sources with unusual properties distinguishing them from both rotation-powered and most accretion-powered pulsar systems. We have studied the temporal and spectral properties of a near-complete sample of these objects using archival ASCA data in the energy range 0.5-10.0 keV. We discuss the characteristics of the spectra and lightcurves of the objects, and the implications for the various theoretical models of SGRs and AXPs.

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