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Ultraviolet studies of stars in the populous cluster NGC 2100 in the Large Magellanic CloudThe ultraviolet energy distributions of the B stars in the LMC cluster NGC 2100 have been studied. The ultraviolet extinction law was studied for the LMC cluster. The T(eff)-luminosity diagrams were determined. The brightest stars in the cluster are evolved stars on the 'horizontal' supergiant branch. No P Cygni profiles indicating mass loss were recognized for these supergiants.
Document ID
19850053262
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/163138
Authors
Bohm-Vitense, E. (Washington Univ. Seattle, WA, United States)
Proffitt, C. (Washington, University Seattle, WA, United States)
Hodge, P. (Observatorio Interamericano de Cerro Tololo, La Serena, Chile; Washington, University Seattle, WA, United States)
Date Acquired
August 12, 2013
Publication Date
May 1, 1985
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 292
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
85A35413
Funding Number(s)
CONTRACT_GRANT: NAG5-207
Distribution Limits
Public
Copyright
Other

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