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HI Study of Southern Galactic Supernova Remnants

Published online by Cambridge University Press:  19 July 2016

Bon-Chul Koo
Affiliation:
SEES, Seoul National University, Seoul 151-742, Korea
Ji-hyun Kang
Affiliation:
SEES, Seoul National University, Seoul 151-742, Korea
Naomi McClure-Griffiths
Affiliation:
ATNF, CSIRO, P.O. Box 76, Epping NSW 1710, Australia

Abstract

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We briefly summarize the survey of HI 21 cm emission lines to search for shocked atomic gas associated with Galactic supernova remnants (SNRs) in the southern sky. For G347.3–0.5, we discuss the distance to the SNR and the implications of the HI results.

Type
Part 2: Supernova Remnants
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Dame, T. M., Hartmann, D., & Thaddeus, P. 2001, ApJ, 547, 792.CrossRefGoogle Scholar
Koo, B.-C., & Heiles, C. 1991, ApJ, 382, 204.Google Scholar
Koyama, K., Kinugasa, K., Matsuzaki, K., Nishiuchi, M., Sugizaki, M., Torii, K., Yamauchi, S., & Aschenbach, B. 1997, PASJ, 49, L7.Google Scholar
Muraishi, H., et al. 2000, A&A, 354, L57.Google Scholar
Slane, P., Gaensler, B. M., Dame, T. M., Hughes, J. P., Plucinsky, P. P., & Green, A. 1999, ApJ, 525, 357.Google Scholar