XMM-Newton Proposal 02061101

Details XMM-Newton Proposal 02061101 XMM-Newton Proposal 02061101

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..317i&link_type=abstract

XMM-Newton Proposal ID #02061101

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Exo 1912+097, Xmm-Newton Proposal 02061101

Scientific paper

The BeppoSAX Wide Field Cameras observations yielded a number of sources which, if at the canonical 8 kpc distance, are less luminous than 10**36 erg/s. Some of these are transients, while others appear to be persistent. Most likely, many of these are high-mass X-ray binaries. One case concerns EXO 1912+097. The prime objectives of the XMM-Newton observation proposed here are to investigate the broad emission feature in detail and understand the nature of the source (i.e., through a search for a slow pulsar and variations in N(H)). A secondary objective is to determine a more accurate position to facilitate optical investigations.

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