Physics
Scientific paper
Sep 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cxo..prop.2137c&link_type=abstract
Chandra Proposal ID #08400666
Physics
Chandra Proposal Id #08400666
Scientific paper
We propose to observe four neutron star (NS) soft X-ray transients in outburst to obtain accurate source positions, continuing a successful program from the previous 2 cycles. This continuing study will allow us to reobserve such sources in future cycles to study the quiescent X-ray emission in NS SXTs. Recent results from Chandra and XMM suggest that the standard picture of NS SXT emission may not be as straightforward as previously thought. This proposal will increase the number of known SXTs with good positions, providing a more uniform sample of the population for future work.
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