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Central Compact Objects in Supernova Remnants

George G. Pavlov (Pennsylvania State University), Divas Sanwal (Pennsylvania State University), Marcus A. Teter (Pennsylvania State University)

arXiv: astro-ph/0311526v1 (astro-ph)

8 pages, 2 figures, newpasp.sty. To appear in "Young Neutron Stars and Their Environments" (IAU Symposium 218, ASP Conf. Proc.), eds F. Camilo and B. M. Gaensler. A typo corrected

Abstract: There are point-like sources in central regions of several supernova remnants which have not been detected outside the X-ray range. The X-ray spectra of these Central Compact Objects (CCOs) have thermal components with blackbody temperatures of 0.2-0.5 keV and characteristic sizes of 0.3-3 km. Most likely, the CCOs are neutron stars born in supernova explosions. We overview their observational properties, emphasizing the Chandra data, and compare them with magnetars.

Submitted to arXiv on 23 Nov. 2003