Wolf-Rayet stars in the Magellanic Clouds release_m4icttsoubakbazunc7zc6nrue

by Lindsey F. Smith

Published in Symposium - International astronomical union by Cambridge University Press (CUP).

1991   Volume 148, p267-272


The most striking feature of the Wolf-Rayet stars in the Magellanic Clouds is their subtype distribution. The range of WC subtypes found in the Large and Small Cloud agrees with evolutionary model predictions at the corresponding metallicities. It follows that the WR subtype distribution in any external galaxy is a clear indicator of the metallicity in that galaxy.The fluxes in the emission lines of WC stars appear to be consistent within the LMC. This can be used (with some precautions) in the Milky Way and other galaxies to determine reddening, distance and the numbers of WR stars in compact regions.
In application/xml+jats format

Archived Files and Locations

application/pdf  757.7 kB
web.archive.org (webarchive)
www.cambridge.org (web)
Read Archived PDF
Type  article-journal
Stage   published
Year   1991
Language   en ?
Container Metadata
Not in DOAJ
In Keepers Registery
ISSN-L:  0074-1809
Work Entity
access all versions, variants, and formats of this works (eg, pre-prints)
Catalog Record
Revision: 13f4d9ab-5f5a-4227-b03d-6a108e54047e