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2002ApJ...566.1039M - Astrophys. J., 566, 1039-1044 (2002/February-3)
Is the compact source at the center of Cassiopeia A pulsed?
MURRAY S.S., RANSOM S.M., JUDA M., HWANG U. and HOLT S.S.
Abstract (from CDS):
A 50 ks Advanced CCD Imaging Spectrometer (ACIS) observation was taken, and analysis of these data for the central object shows that the spectrum is consistent with several forms and that the emitted X-ray luminosity in the 0.1-10 keV band is 1033-1035 ergs.cm–2.s–1, depending on the spectral model and the interstellar absorption along the line of sight to the source. The spectral results are consistent with those of Pavlov et al. and Chakrabarty et al.
Abstract Copyright: ∼
Journal keyword(s): ISM: individual (Cassiopeia A) - Stars: Pulsars: General - Stars: Neutron - ISM: Supernova Remnants - X-Rays: Stars
Simbad objects: 5
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