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A young association in the Large Magellanic Cloud

Published online by Cambridge University Press:  14 August 2015

B. J. Bok
B. J. Bok*
Affiliation:
Mount Stromlo Observatory

Extract

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During the past three years, Priscilla F. Bok, Jane Basinski, and I have concentrated in our work on the Large Magellanic Cloud upon the study of young associations. One colour-magnitude array, that of NGC 1955–68–74, has been published (Bok, Bok, and Basinski 1962), and work on three additional groupings, NGC 1929–34–35–36–37, NGC 1770, and NGC 1814–16–20 is well under way. We shall report here on NGC 1929–37, which is often referred to as “Shapley's Constellation I”. Its position is α = 5h22m0; δ = −68°00′ (1960).

Type
Section II: The Magellanic Clouds
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 335 - 342
Copyright
Copyright © Australian Academy of Science 1964 

References

Blaauw, A. (1958).—“Stellar Populations.” [Vatican City 1957.] (Ed. O'Connell, D. J. K..) (North Holland Publishing Co.: Amsterdam.)Google Scholar
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Bok, B. J., Bok, P. F., and Basinski, J. M. (1962).— M.N. 123: 487–96 = Mount Stromlo Obs. Reprint No. 51.Google Scholar
Doherty, L., Henize, K. G., and Aller, L. H. (1956)— Ap. J. Suppl. 2: 345–63.Google Scholar
Feast, M. W., Thackeray, A. D., and Wesselink, .A. J. (1960).—M.N. 121: 337–85 = Radcliffe Obs. Comm. No. 55.Google Scholar
Limber, D. N. (1960).— Ap. J. 131: 168–201.Google Scholar
Westerlund, B. E. (1961).— Uppsala Astron. Obs. Annaler 5 No. 1.Google Scholar