Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-25T17:05:59.738Z Has data issue: false hasContentIssue false
  • English
  • Français

Supernova Remnants in the UWISH2 and UWIFE Surveys

Published online by Cambridge University Press:  29 January 2014

Yong-Hyun Lee ,
Bon-Chul Koo  and
Jae-Joon Lee
Yong-Hyun Lee
Affiliation:
Department of Physics and Astronomy, Seoul National University, 1 Gwanak-ro, Gwanak-gu, Seoul 151-742, Republic of Korea email: [email protected], [email protected]
Bon-Chul Koo
Affiliation:
Department of Physics and Astronomy, Seoul National University, 1 Gwanak-ro, Gwanak-gu, Seoul 151-742, Republic of Korea email: [email protected], [email protected]
Jae-Joon Lee
Affiliation:
Korea Astronomy and Space Science Institute, 776, Daedeokdae-ro, Yuseong-gu, Daejeon, Republic of Korea email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Keywords

surveysISM: supernova remnantsinfrared: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S296: Supernova Environmental Impacts , January 2013 , pp. 370 - 371
Copyright
Copyright © International Astronomical Union 2014 

References

Alonso-Herrero, A., Rieke, G. H., Rieke, M. J., & Kelly, D. M. 2003, AJ, 125, 1210CrossRefGoogle Scholar
Diolaiti, E., Bendinelli, O., Bonaccini, D., et al. 2000, A&AS, 147, 335Google Scholar
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