Spectrophotometry of Early-Type Supergiants in the Large Magellanic Cloud

Details Spectrophotometry of Early-Type Supergiants in the Large Magellanic Cloud Spectrophotometry of Early-Type Supergiants in the Large Magellanic Cloud

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..233n&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Physics

Scientific paper

Equivalent widths of major stellar features in the visible and UV
regions of a sample of LMC supergiants whose types range from O5 to A1
have been derived. No systematic differences in these features are
detectable between LMC and galactic O and early B supergiants.

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