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The Compact HII Regions N11A and N88A in the LMC and SMC

Published online by Cambridge University Press:  25 May 2016

G. Testor ,
C. S. Rola  and
A. B. Whiting
G. Testor
Affiliation:
Observatoire de Meudon, 92195 Meudon Cedex, France
C. S. Rola
Affiliation:
Institute of Astronomy, University of Cambridge, United Kingdom
A. B. Whiting
Affiliation:
Physics Department, U.S. Naval Academy, Annapolis, MD 21402, USA

Abstract

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Several spectra have been obtained in the 3600–10000 Å range, for the HII regions N11A and N88A in the LMC and SMC, respectively. The spectral type of their exciting star was determined and from the emission-line intensities we have derived the gas electron density and temperature, and computed the chemical abundances of He, O, N, Ne, S, and Ar. These abundances are then compared with the ones found for other HII regions in the Magellanic Clouds.

Type
Part 2. Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 132 - 133
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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