Spectrophotometry of Early-Type Supergiants in the Large Magellanic Cloud
Abstract
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.
- Publication:
-
Structure and Evolution of the Magellanic Clouds
- Pub Date:
- September 1984
- DOI:
- 10.1017/S0074180900040274
- Bibcode:
- 1984IAUS..108..233N