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The Oxygen-Rich Supernova Remnant in the Small Magellanic Cloud

Published online by Cambridge University Press:  12 April 2016

William P. Blair ,
John C. Raymond ,
John Danziger  and
Francesca Matteucci
William P. Blair
Affiliation:
The Johns Hopkins University, Baltimore, Md., U.S.A
John C. Raymond
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, Ma., U.S.A
John Danziger
Affiliation:
European Southern Observatory, Garching bei Munchen, West Germany
Francesca Matteucci
Affiliation:
European Southern Observatory, Garching bei Munchen, West Germany

Abstract

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We report ultraviolet and optical spectra of IE 0102-7219, the oxygen-rich supernova remnant in the Small Magellanic Cloud. The UV data contain strong lines of oxygen, carbon, neon, and magnesium. OI recombination lines in the optical and UV permit the relative line intensities to be determined from 1200Å to 1 micron. Models assuming shock excitation and X-ray photoionization have been calculated and compared with the observations.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 187 - 190
Copyright
Copyright © Cambridge University Press 1988

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