A New Compact Object / Remnant Association in SNR G292.0+1.8

Details A New Compact Object / Remnant Association in SNR G292.0+1.8 A New Compact Object / Remnant Association in SNR G292.0+1.8

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..262..331o&link_type=abstract

The High Energy Universe at Sharp Focus: Chandra Science, held in conjunction with the 113th Annual Meeting of the ASP. ASP Conf

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a new 100 ks Chandra Observation of the dim supernova remnant 3C396. These data show clear evidence of diffuse (but compact), nebular emission slightly offset from the center of the remnant which interpret as a synchrotron wind nebula surrounding a neutron star that is physically associated with the remnant. We present images and spectra of this new neutron star/supernova remnant association and compare the results to similar objects recently discovered by Chandra.

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