XMM-Newton Proposal 02068801

Details XMM-Newton Proposal 02068801 XMM-Newton Proposal 02068801

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..353m&link_type=abstract

XMM-Newton Proposal ID #02068801

Physics

Rx J1836.2+5925, Xmm-Newton Proposal 02068801

Scientific paper

We propose a 70 ks observation for the X-ray counterpart of an unidentified EGRET source, RX J1836.2+5925. This source is inferred to be a radio-quiet isolated neutron star and a prototype of the Gould Belt sources. Furthermore, the spectral energy distribution from radio to gamma-ray resembles the Geminga, which is as-yet enigmatic radio-quiet gamma-ray pulsar. The goals of our observation are as follows. (1) To measure the spectral parameters precisely. (2) To detect the pulsation to understand this source, the Gould Belt sources and the Geminga. The mechanisms of the radio-quiescence under the models could be tested.

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