Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-19T04:42:51.982Z Has data issue: false hasContentIssue false
  • English
  • Français

2. 21-cm. observations in Sydney

Published online by Cambridge University Press:  14 August 2015

Martha Stahr Carpenter
Martha Stahr Carpenter*
Affiliation:
Cornell University, Ithaca, New York, U.S.A.

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 primary project in the current 21-cm. hydrogen-line work in Sydney is a study of the southern Milky Way by F. J. Kerr, J. V. Hindman, and the author. Earlier observations* made at the Radiophysics Laboratory during 1954 yielded a tentative picture of spiral structure in the southern portion of the conventional galactic plane. That picture, slightly modified by more recent results, is shown in Fig. 1.

Type
Part I: Spectral Line Investigations
Information
Symposium - International Astronomical Union , Volume 4: Radio Astronomy , 1957 , pp. 14 - 18
Copyright
Copyright © Cambridge University Press 1957 

References

1. van de Hulst, H. C., Muller, C. A. and Oort, J. H. B.A.N. 12, 117–49, no. 452, 1954.Google Scholar
2. Edmondson, F. K. P.A.S.P. 67, 10–11, 1955.CrossRefGoogle Scholar