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Supernova Remnants in the UWISH2 and UWIFE Surveys

Published online by Cambridge University Press:  29 January 2014

Yong-Hyun Lee
Affiliation:
Department of Physics and Astronomy, Seoul National University, 1 Gwanak-ro, Gwanak-gu, Seoul 151-742, Republic of Korea email: yhlee@astro.snu.ac.kr, koo@astro.snu.ac.kr
Bon-Chul Koo
Affiliation:
Department of Physics and Astronomy, Seoul National University, 1 Gwanak-ro, Gwanak-gu, Seoul 151-742, Republic of Korea email: yhlee@astro.snu.ac.kr, koo@astro.snu.ac.kr
Jae-Joon Lee
Affiliation:
Korea Astronomy and Space Science Institute, 776, Daedeokdae-ro, Yuseong-gu, Daejeon, Republic of Korea email: leejjoon@kasi.re.kr
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Abstract

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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

Alonso-Herrero, A., Rieke, G. H., Rieke, M. J., & Kelly, D. M. 2003, AJ, 125, 1210CrossRefGoogle Scholar
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Froebrich, D., Davis, C. J., Ioannidis, G., et al. 2011, MNRAS, 413, 480CrossRefGoogle Scholar
Green, D. A. 2009, Bulletin of the Astronomical Society of India, 37, 45Google Scholar
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