Physics
Scientific paper
Sep 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cxo..prop.2367a&link_type=abstract
Chandra Proposal ID #09400380
Physics
Chandra Proposal Id #09400380
Scientific paper
4U~1850--087 is a candidate ultra-compact X-ray binary. A soft excess near 0.7 keV has been reported for this source with ASCA and interpreted as due to neutral Ne-rich material local to the binary. Recent XMM-Newton and Chandra observations of the source at low X-ray luminosity do not confirm the ASCA results and therefore different physical interpretations are possible. We propose at 30 ks Chandra LETGS observation of this source during its high luminosity state in order to understand how the luminosity affects the abundances observed in the X-ray spectrum.
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