Physics
Scientific paper
Mar 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop....5k&link_type=abstract
XMM-Newton Proposal ID #02000701
Physics
4U 1636-536, Xmm-Newton Proposal 02000701
Scientific paper
The discovery of millisecond variability in the hard (2.5-30 keV) emission of neutron-star low-mass x-ray binaries opened a new window on the study of the accretion flow and the effects of strong gravitational fields in these systems. We plan to use XMM-Newton to search for millisecond variability in the soft x-ray band (0.4-2.5 keV), which is inaccessible to RXTE, from sources which have shown kHz quasiperiodic oscillations (QPOs) in hard x-rays. This observations will place important constraints on models of the kHz QPOs.
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