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A study of bright members of the large magellanic cloud

Published online by Cambridge University Press:  27 June 2016

M. W. Feast ,
A. D. Thackeray  and
A. J. Wesselink
M. W. Feast
Affiliation:
Radcliffe Observatory, Pretoria, South Africa
A. D. Thackeray
Affiliation:
Radcliffe Observatory, Pretoria, South Africa
A. J. Wesselink
Affiliation:
Radcliffe Observatory, Pretoria, South Africa

Extract

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A progress report on work on (a) spectral types and (b) radial velocities of twenty-eight members of the Large Cloud (mostly mpg = 11 or brighter) will appear shortly in The Observatory. The commonest spectral types found lie between B 5 and A 2. A star with Mpg= − 10·1 has slightly narrower H-lines than the galactic A 2 super-giant HD 92207. [Fe 11] emission appears in four of the stars, including recent spectra of S Dor.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 5: The Large-Scale Structure of the Galactic System , 1958 , pp. 7
Copyright
Copyright © Cambridge University Press 1958