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The ISM near SN 1987A: Kinematics and 3-D Structure

Published online by Cambridge University Press:  25 May 2016

Arlin P.S. Crotts  and
Jun Xu
Arlin P.S. Crotts
Affiliation:
Dept. of Astronomy, Columbia University, New York, NY 10027, USA
Jun Xu
Affiliation:
Dept. of Astronomy, Columbia University, New York, NY 10027, USA

Abstract

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We present two views of the region around SN 1987A: a three-dimensional map of structure revealed by light echoes, and a multicomponent velocity map at 10 km s−1 resolution in [N II], correlating the various superbubble structures found in both, with implications for their age and dynamics, as well as the history of the SN progenitor.

Type
Part 2. Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 162 - 164
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Kim, S., et al. 1998, ApJ, 503, 674 CrossRefGoogle Scholar
McCray, R., & Kafatos, M. 1987, ApJ, 317, 190 CrossRefGoogle Scholar
Wang, Q., & Helfand, D.J. 1991a, ApJ, 370, 541 CrossRefGoogle Scholar
Wang, Q., & Helfand, D.J. 1991b, ApJ, 373, 497 CrossRefGoogle Scholar
Xu, J., & Crotts, A.P.S. 1999, ApJ, 511, 262 CrossRefGoogle Scholar
Xu, J., Crotts, A.P.S., & Kunkel, W.E. 1995, ApJ, 451, 806 (Erratum: 463, 391) Google Scholar