C H A N D R A
S C I E N C E
C E N T E R O B S E R V A T I O N C A T A L O G |
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Abstract: Previous studies of the young (340 yr) Central Compact Object (CCO) in the Cas A supernova remnant resulted in a reported decrease of the CCO's surface temperature by about 2% in 10 years. However, the actual rate of this exceptional cooling is still uncertain as the most recent data hint at a puzzling difference between cooling trends in early and later years. In order to constrain the cooling rate more accurately, we propose to continue the monitoring of the thermal evolution of this neutron star. The legacy time series of the Cas A CCO provides a crucial checkpoint for theoretical models concerning the properties of the neutron star interior. |
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