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Analysis of Multiwavelength Observations of IC443

Published online by Cambridge University Press:  12 April 2016

M.L. McColloug  and
S.L. Mufson
M.L. McColloug
Affiliation:
Physics Department, Oklahoma State University Astronomy Department, Indiana University
S.L. Mufson
Affiliation:
Astronomy Department, Indiana University

Abstract

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High resolution observations at radio, infrared, optical and X-ray wavelengths have been made (Mufson et al. 1986). The infrared spectrum determined from the IRAS observations has been fitted with models which include shock heated dust, infrared line emission, and radiatively heated dust emission. Numerical simulations of a supernova expanding into a uniform medium, which describe the X-ray and large scale radio emission, are presented.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 403 - 406
Copyright
Copyright © Cambridge University Press 1988

References

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Wolff, M.J., 1986. Ph.D. Dissertation, Indiana University.Google Scholar