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Spectrophotometry of six high-excitation compact H II regions in the Magellanic Clouds

Published online by Cambridge University Press:  26 May 2016

Gérard Testor*
Affiliation:
Laboratoire de l'Univers et de ses Theories, Observatoire de Paris-Meudon, F-92195 Meudon, la France

Abstract

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Series of CCD long-slit spectra have been obtained in the 3600-10000 Å range, with the ESO 1.5m telescope, for the six brightest compact H ii regions in the LMC and SMC: N 11A, N 160 A1-A2 and N 88A, N 81 and N 26A-B, respectively. For each region the spectral type of its complex exciting source is given. 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, which we compare with the ones found for other H ii regions in the Magellanic Clouds.

Type
Part 4. Feedback from Massive Stars
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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