XMM-Newton Proposal 03045307

Details XMM-Newton Proposal 03045307 XMM-Newton Proposal 03045307

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..154p&link_type=abstract

XMM-Newton Proposal ID #03045307

Computer Science

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, 1E 1207.4-5209, 1E 1207.4-5209, 1E 1207.4-5209, 1E 1207.4-5209, 1E 1207.4-5209, 1E 1207.4-5209, 1E 1207.4-5209, Xmm-Newton Proposal 03045307

Scientific paper

Chandra and XMM observations of 1E 1207.4-5209, the central compact object in the SNR PKS 1209--51/52, led to the discoveries of its 424 ms spin period and prominent absorption lines in its thermal-like X-ray spectrum, which provided an exciting opportunity to measure the gravitational redshift at the surface of a neutron star. These observations, spread over a 3.5 yr period, have also revealed an intriguing nonmonotonous behavior of the spin period. To understand the nature of this enigmatic object, we propose a series of observations with the XMM EPIC detectors.

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