Deep Crustal Heating and Quasi-Persistent Transients

Details Deep Crustal Heating and Quasi-Persistent Transients Deep Crustal Heating and Quasi-Persistent Transients

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1068..185b&link_type=abstract

A DECADE OF ACCRETING MILLISECOND X-RAY PULSARS. AIP Conference Proceedings, Volume 1068, pp. 185-190 (2008).

Computer Science

1

Neutron Stars, X-Ray Binaries, Pulsars

Scientific paper

Accreting millisecond pulsars provide a glimpse into the thermal, chemical, and magnetic evolution of accreting neutron stars. In this contribution I review how accretion-induced nuclear processes alter the composition of the neutron star crust and heat the neutron star core; how observations of quasi-persistent transient neutron stars probe the equation of state of dense matter; and how these observations compare with complimentary studies of quasi-persistent transients and superbursting neutron stars.

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