Other
Scientific paper
Mar 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop...42s&link_type=abstract
XMM-Newton Proposal ID #02008201
Other
X1832-330, Xmm-Newton Proposal 02008201
Scientific paper
ASCA and BeppoSAX observations of a number of ultra-compact (orbital period less than 1hr) X-ray binaries have revealed two possible spectral differences compared to other LMXRB systems. These are (1) the presence of a discrete feature near 0.7 keV (attributed to Ne) and (2) their best-fit parameter values when fit with a disk-blackbody and Comptonized continuum. We wish to clarify and extend the emerging picture of a spectral signature for the ultra-compact systems usign XMM-Newton. The proposed observation will allow a clear confirmation of such a signature which will, in turn, allow the nature of a LMXRB to be determined from its spectral characteristics.
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