Physics
Scientific paper
Sep 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.1939c&link_type=abstract
Chandra Proposal ID #07400737
Physics
Chandra Proposal Id #07400737
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 we initiated in Cycle 6. 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 stadard 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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