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Interstellar Dust in the LMC

Published online by Cambridge University Press:  04 August 2017

Geoffrey C. Clayton  and
Peter G. Martin
Geoffrey C. Clayton
Affiliation:
Department of Astronomy, University of Toronto
Peter G. Martin
Affiliation:
Department of Astronomy, University of Toronto

Abstract

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New IUE observations confirm the differences between the Galactic and LMC ultraviolet extinction curves and show some evidence for variations within the LMC. Visual and infrared photometry and polarimetry show that the anomalous properties of the LMC dust do not extend to longer wavelengths. Despite the much different dust to gas ratios in the Galaxy and the Magellanic clouds, the dust formation efficiency is similar when the abundances are included.

Type
Interstellar Matter
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 403 - 404
Copyright
Copyright © Reidel 1984 

References

Bromage, G.E., and Nandy, K. 1983, Monthly Notices Roy. Astron. Soc. 204, pp. 29p.Google Scholar
Clayton, G.C., Martin, P.G., and Thompson, I. 1983, Astrophys. J. 265, 194 CrossRefGoogle Scholar
Dufour, R.J., Shields, G.A., and Talbot, R.J. 1982, Astrophys. J. 252, pp. 461.Google Scholar
Koornneef, J. 1982, Astron. Astrophys. 107, 247 Google Scholar
Massa, D., and Savage, B.D. 1983, preprint.Google Scholar