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A Comparison of Radio and Optical Observations of the 30 Doradus Nebula

Published online by Cambridge University Press:  25 April 2016

A. E. Le Marne
A. E. Le Marne*
Affiliation:
School of Physics, University of Sydney
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Extract

The Sydney University one mile cross-type radio telescope at the Molonglo Radio Observatory has been used to study the 30 Doradus nebula with high resolution (~3´ arc) at 408 MHz. This preliminary report compares these observations with Balmer line isophotes published by Faulkner. A description of the calibration procedures used in the present observations, an analysis of the various radio features in the 30 Doradus region, and a comparison with previous observations at other frequencies, will be described in a later paper.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 3 , February 1968 , pp. 97 - 98
Copyright
Copyright © Astronomical Society of Australia 1968

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References

1 Faulkner, D.J., M.N.R.A.S., 135, 401 (1967).Google Scholar
2 Feast, M.W., Thackeray, A.D., and Wesselink, A.J., M.N.R.A.S., 121, 337 (1960).Google Scholar
3 Johnson, H.L., Astrophys. J., 147, 912 (1967).Google Scholar
4 Mills, B.Y., and Shaver, P.A., Aust. J. Phys., in press.Google Scholar