Hostname: page-component-848d4c4894-sjtt6 Total loading time: 0 Render date: 2024-07-03T15:20:31.862Z Has data issue: false hasContentIssue false

A study of bright members of the large magellanic cloud

Published online by Cambridge University Press:  27 June 2016

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Copyright
Copyright © Cambridge University Press 1958