Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-25T16:51:12.812Z Has data issue: false hasContentIssue false
  • English
  • Français

The Scorpio–Centaurus association

Published online by Cambridge University Press:  14 August 2015

A. Blaauw
A. Blaauw*
Affiliation:
Kapteyn Astronomical Laboratory, Groningen

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.

The Scorpio–Centaurus association extends from about lII=356°, bII=+20° towards lower longitudes over about 90° of the southern sky. Between lII=312 and 356° it is located between latitudes +10 and +25°, and appears well detached from the more distant B-star population at lower latitudes. At longitudes below 312° it approaches and crosses the galactic plane and is seen projected against the general low latitude B-star population from which it is more difficult to separate. These features are clearly brought out by Figures 5 and 6 of the author's thesis (1946) and had been recognized earlier by others (e.g. Kapteyn 1914).

Type
Section 1: The Galaxy
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 50 - 56
Copyright
Copyright © Australian Academy of Science 1964 

References

Bertiau, F. C. (1958).— Ap. J. 128: 533–61 (=McDonald Contr. No. 291).Google Scholar
Blaauw, A. (1946).—Publ. Kapteyn Astron. Laboratory No. 52.Google Scholar
Blaauw, A. (1963).—“Stars and Stellar Systems.” (General Ed. Kuiper, G. P..) vol. III. Chapter 20. (Univ. Chicago Press.)Google Scholar
Borgman, J. (1960).— B.A.N. 15: 255–63.Google Scholar
Eggen, O. J. (1961).—Royal Obs. Bull. No. 41.Google Scholar
Hardie, R. H., and Crawford, D. L. (1961).— Ap. J. 133: 843–59.Google Scholar
Kapteyn, J. C. (1914).— Ap. J. 40: 43–126 (= Mount Wilson Contr. No. 82).CrossRefGoogle Scholar
Petrie, R. M. (1962).— M.N. 123: 501–8.Google Scholar
Walraven, Th., and Walraven, J. H. (1960).— B.A.N. 15: 67–83.Google Scholar