XMM-Newton Proposal 02037003

Details XMM-Newton Proposal 02037003 XMM-Newton Proposal 02037003

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..192t&link_type=abstract

XMM-Newton Proposal ID #02037003

Computer Science

Psr J1301-6310, Psr J1849-0317, Psr J1530-5327, Xmm-Newton Proposal 02037003

Scientific paper

Middle-aged pulsars (10-100 kyr) provide the opportunity to study the thermal X-ray radiation from neutron stars (NSs). Their observations, combined with the NS cooling models, have the potential to constrain the nature of the superfluid interior, the composition of the stellar core, the processes responsible for the NS cooling, and the NS mass and radius. We propose to observe three nearby middle-aged pulsars discovered recently in the Parkes Multibeam Pulsar Survey: PSR J1301--6310, J1849--0317, and J1530--5327. These observations will allow us to measure the spectral parameters and study the thermal component of the pulsars radiation, which will help to constrain the NS thermal evolution models.

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