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Supernova Remnants in the UWISH2 and UWIFE Surveys

  • Yong-Hyun Lee (a1), Bon-Chul Koo (a1) and Jae-Joon Lee (a2)

Abstract

We report the preliminary results for the detection of H2 and [Fe II] line features around the Galactic supernova remnants (SNRs) from the UWISH2 and UWIFE surveys that cover the first galactic quadrant of 7°<l<65° and |b|<1.3°. By this time, we have found a total of 17 H2-emitting and 14 [Fe II]-emitting SNRs in the coverage, and more than a half of them are detected in both H2 and [Fe II] emissions, which implies that the environment of these SNRs might be complex and composed of multi-phase medium. In this paper, we present our identification strategy and some preliminary results including H2 and [Fe II] luminosity distributions.

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Alonso-Herrero, A., Rieke, G. H., Rieke, M. J., & Kelly, D. M. 2003, AJ, 125, 1210
Diolaiti, E., Bendinelli, O., Bonaccini, D., et al. 2000, A&AS, 147, 335
Froebrich, D., Davis, C. J., Ioannidis, G., et al. 2011, MNRAS, 413, 480
Green, D. A. 2009, Bulletin of the Astronomical Society of India, 37, 45
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