Department - Author 1

Physics Department

Degree Name - Author 1

BS in Physics

Date

3-2010

Primary Advisor

Michelle Ouellette

Abstract/Summary

Central compact objects (CCOs) are point-like sources found near the center of supernova remnants (SNRs). They emit X-rays, but show no radio or gamma ray counterpart. Typical CCO candidates have emission radii on the order of 0.2-3.0 km. This is much smaller than the typical radius of a neutron star, making CCOs a difficult astronomical phenomenon to identify.

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