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Interstellar Abundances in the Magellanic Clouds

Published online by Cambridge University Press:  25 May 2016

D. E. Welty,
P. C. Frisch,
L. M. Hobbs,
D. G. York,
J. C. Blades,
J. T. Lauroesch and
G. Sonneborn
D. E. Welty
Affiliation:
University of Chicago, 5640 S. Ellis Ave., Chicago, IL 60637, USA
P. C. Frisch
Affiliation:
University of Chicago, 5640 S. Ellis Ave., Chicago, IL 60637, USA
L. M. Hobbs
Affiliation:
University of Chicago, 5640 S. Ellis Ave., Chicago, IL 60637, USA
D. G. York
Affiliation:
University of Chicago, 5640 S. Ellis Ave., Chicago, IL 60637, USA
J. C. Blades
Affiliation:
STScI, 3700 San Martin Dr., Baltimore, MD 20771, USA
J. T. Lauroesch
Affiliation:
Northwestern University, Evanston, IL 60208, USA
G. Sonneborn
Affiliation:
Goddard Space Flight Center, Code 681, Greenbelt, MD 21218, USA

Abstract

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We discuss the relative gas-phase abundances found for the predominantly neutral interstellar clouds — located in the Galactic disk and halo, in the LMC or SMC, and (perhaps) in between — along the lines of sight to Sk 108 in the SMC and to SN 1987A in the LMC.

Information

Type
Part 4. Detailed Chemical Abundances
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999, pp. 277 - 278
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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