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Limits on the Presence of Sulfur in the Young SNRs LMC N132D and SMC 1E0102.2-7219

Published online by Cambridge University Press:  12 April 2016

Barry M. Lasker
Barry M. Lasker*
Affiliation:
Space Telescope Science Institute, Baltimore, MD, USA

Abstract

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A new area-spectroscopy search for sulfur as a tracer of the “Si Group” of elements in the ejecta of the young SNRs, LMC N132D and SMC 1E0102.2–7219, yields negative results for [S II]λλ6719, 6731 and [S III]λλ9064, 9532.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 191 - 192
Copyright
Copyright © Cambridge University Press 1988

References

Dopita, M.A., and Tuohy, L.R. 1984 Ap.J., 282, 135.CrossRefGoogle Scholar
Johnston, M.D., and Yahil, A. 1984 Ap.J., 285, 587.Google Scholar
Lasker, B.M. 1980, Ap.J., 237, 765.CrossRefGoogle Scholar
Winkler, P.F., and Kirshner, R.P. 1985 Ap.J., 299, 981.Google Scholar