XMM-Newton Studies of the Remarkable Binary Millisecond Pulsar PSR J1614-2230

Details XMM-Newton Studies of the Remarkable Binary Millisecond Pulsar PSR J1614-2230 XMM-Newton Studies of the Remarkable Binary Millisecond Pulsar PSR J1614-2230

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..176r&link_type=abstract

XMM-Newton Proposal ID #04047901

Computer Science

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Psr J1614-2230, Xmm-Newton Proposal 04047901

Scientific paper

The 3.15 ms pulsar PSR J1614-2230 was discovered during a recent radio survey of unidentified EGRET gamma-ray sources. It is the first true millisecond pulsar detected with a companion whose minimum mass is ~0.4 solar. A short (5 ks), exploratory XMM-Newton observation revealed it to be an X-ray source with an apparent extended nebular trail. Here we request a deeper, 50 ks, observation with XMM-Newton to determine the spectra of the two X-ray components and to search for structure on larger scales.

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