Physics
Scientific paper
Sep 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2361c&link_type=abstract
Chandra Proposal ID #09400192
Physics
Chandra Proposal Id #09400192
Scientific paper
We propose a 30 ksec observation of each of the quasi-persistent neutron-star low-mass X-ray transients KS 1731-260 and MXB 1659-29 in quiescence. The long outbursts in both of these sources heated the neutron star crust out of thermal equilibrium with the core. We have tracked the cooling of the neutron star crusts in both objects since they went in quiescence. We have preliminary evidence that the cooling has ceased, perhaps indicating that the crust is in equilibrium with the core. Our proposed observations will test the equilibrium suggestion, by placing tight limits on residual cooling and/or residual accretion, and determine the core temperature, constraining the equation of state of dense matter.
No associations
LandOfFree
Crustal cooling in quiescent neutron stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Crustal cooling in quiescent neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Crustal cooling in quiescent neutron stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-964907