The Cold Dust Content of the Oxygen-Rich Supernova Remnant G292.0+1.8

11 Aug 2016 Ghavamian Parviz Williams Brian J.

We present far-infrared images of the Galactic oxygen-rich supernova remnant (SNR) G292.0+1.8, acquired with the PACS and SPIRE instruments of the Herschel Space Observatory. We find that the SNR shell is detected in the PACS blue (100 micron) band, but not in the red (160 micron) band, broadly consistent with results from AKARI observations... (read more)

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  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • ASTROPHYSICS OF GALAXIES