A Morphological Analysis of the Supernova Remnant G292.0+1.8 with Chandra and ATCA

Details A Morphological Analysis of the Supernova Remnant G292.0+1.8 with Chandra and ATCA A Morphological Analysis of the Supernova Remnant G292.0+1.8 with Chandra and ATCA

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..262..343j&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 archival Chandra images of the Galactic SNR G292.0+1.8.
G292.0+1.8 is a bright, young, oxygen-rich SNR, with a prominent
embedded point source which is likely a pulsar wind nebula (Olbert et
al., this meeting). We present narrow-band and continuum images, as well
as spectral analysis of selected regions

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