Supernova Remnants In The Chasem33 X-ray Observations Of M33

Mathematics – Logic

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Scientific paper

M33 contains at least 100 SNRs identified from optical emission-line and radio imaging studies. Many of these SNRs have been detected with Chandra in the ChASeM33 study of that galaxy, several with enough S/N to carry out detailed spectral analysis. Here we report the results of our search for SNRs in the entire multi-wavelength data set, including our Chandra survey, new radio observations from the VLA, and new optical spectroscopy, as well as existing optical, radio, and X-ray data on M33. We have developed a morphological classification scheme for the optically-identified SNRs; we will discuss whether this scheme is a good predictor of X-ray detectability. Finally, we compare the SNRs found in M33 to those that have been observed in the Galaxy and the Magellanic Clouds, in order to assess whether we might still be missing young SNRs like Cas A, Tycho's SNR or the Crab Nebula in M33.

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