Confirming the Structure of the Nebular Trail of PSR J1614-2230

Details Confirming the Structure of the Nebular Trail of PSR J1614-2230 Confirming the Structure of the Nebular Trail of PSR J1614-2230

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cxo..prop.2143r&link_type=abstract

Chandra Proposal ID #08400891

Computer Science

Chandra Proposal Id #08400891

Scientific paper

The 3.15ms 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 as large as 0.4 solar masses. A short (5ks), exploratory XMM-Newton observation revealed it to be an X-ray source with an apparent extended nebular trail. Here we request a 20ks Chandra ACIS-S observation to image the structure of the nebular trail which will complement spectral studies to be performed with an already accepted deeper (50ks) observation by XMM-Newton.

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