Temporal Evolution of Transient Type i Bursters in Quiescence

Details Temporal Evolution of Transient Type i Bursters in Quiescence Temporal Evolution of Transient Type i Bursters in Quiescence

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..587b&link_type=abstract

Chandra Proposal ID #02400714

Physics

Chandra Proposal Id #02400714

Scientific paper

In transiently accreting neutron stars (NSs), the NS crusts are heated during the accretion outbursts. The timescale on which this heat is radiated away after outburst depends on the depth where this heat is deposited. In deep crustal heating, the relevant depths have thermal timescales of days -- years, with most being radiated on a 2 yr timescale. We request observations to observe transient NSs soon after they return to quiescence, to observe this evolution. This proposal is a resubmission of a partially granted ToO proposal which was not triggered during AO1.

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