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Paper: A Morphological Analysis of the Supernova Remnant G292.0+1.8 with Chandra and ATCA
Volume: 262, The High Energy Universe at Sharp Focus: Chandra Science
Page: 343
Authors: Jin, S.; Waite-Jones, C. G.; Keohane, J. W.; Olbert, C. M.; Gaensler, B. M.; Wallace, B. J.
Abstract: 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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