The Central X-Ray Point Source in Cassiopeia A
Abstract
The spectacular ``first light'' observation by the Chandra X-Ray Observatory revealed an X-ray point source near the center of the 300 yr old Cas A supernova remnant. We present an analysis of the public X-ray spectral and timing data. No coherent pulsations were detected in the Chandra/HRC data. The 3 σ upper limit on the pulsed fraction is less than 35% for P>20 ms. The Chandra/ACIS spectrum of the point source may be fitted with an ideal blackbody (kT=0.5 keV) or with blackbody models modified by the presence of a neutron star atmosphere (kT=0.25-0.35 keV), but the temperature is higher and the inferred emitting area lower than expected for a 300 yr old neutron star according to standard cooling models. The spectrum may also be fitted with a power-law model (photon index Γ=2.8-3.6). Both the spectral properties and the timing limits of the point source are inconsistent with a young Crab-like pulsar but are quite similar to the properties of the anomalous X-ray pulsars. The spectral parameters are also very similar to those of the other radio-quiet X-ray point sources in the supernova remnants Pup A, RCW 103, and PKS 1209-52. Current limits on an optical counterpart for the Cas A point source rule out models that invoke fallback accretion onto a compact object if fallback disk properties are similar to those in quiescent low-mass X-ray binaries. However, the optical limits are marginally consistent with plausible alternative assumptions for a fallback disk. In this case, accreting neutron star models can explain the X-ray data, but an accreting black hole model is not promising.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- February 2001
- DOI:
- 10.1086/318994
- arXiv:
- arXiv:astro-ph/0001026
- Bibcode:
- 2001ApJ...548..800C
- Keywords:
-
- Accretion;
- Accretion Disks;
- Black Hole Physics;
- Stars: Neutron;
- supernovae: individual (Cassiopeia A);
- ISM: Supernova Remnants;
- X-Rays: Stars;
- Astrophysics
- E-Print:
- 17 pages including 2 figs. To appear in ApJ, Vol. 546 (Jan 10, 2001). Minor revisions per referee. Pulsation limits revised in light of HRC wiring problem. Typos corrected