Hostname: page-component-84b7d79bbc-4hvwz Total loading time: 0 Render date: 2024-07-26T06:36:25.556Z Has data issue: false hasContentIssue false

The space distribution of the OB-type stars in Carina

Published online by Cambridge University Press:  14 August 2015

J. A. Graham*
Affiliation:
Cerro Tololo Inter-American Observatory, La Serena, Chile

Abstract

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.

Distances have been determined for 436 OB-type stars in Carina. A sharp outside edge is found to the OB star distribution with respect to the center of the Galaxy. The layer of OB stars follows the galactic plane to distances of the order of 3 kpc, but at distances greater than 4 kpc it appears to bend away from the plane to negative latitudes by 2° or 3° out to distances of the order of 10 kpc.

Type
Part II/Observations of Spiral Structure in Our Galaxy
Copyright
Copyright © Reidel 1970 

References

Fernie, J. D.: 1965, Astron. J. 70, 575.CrossRefGoogle Scholar
Graham, J. A.: 1967, Monthly Notices Roy. Astron. Soc. 135, 377.CrossRefGoogle Scholar
Graham, J. A. and Lyngå, G.: 1965, Mem. Mt Stromlo Obs. 4, 16.Google Scholar
The, Pik-Sin: 1966, Contr. Bosscha Obs., 35.Google Scholar
Walraven, T.: 1966, IAU Symposium No. 24, p. 274.CrossRefGoogle Scholar
Walraven, T. and Walraven, J. H.: 1960, Bull. Astron. Inst. Netherl. 15, 67.Google Scholar
Wray, J. R.: 1967, Ph.D. Thesis, Northwestern University.Google Scholar