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HI in the Small Magellanic Cloud Re-examined — II

Published online by Cambridge University Press:  25 April 2016

R.X. McGee  and
Lynette M. Newton
R.X. McGee
Affiliation:
Division of Radiophysics, CSIRO, Sydney
Lynette M. Newton
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

The reasons for re-surveying the neutral hydrogen in the Small Magellanic Cloud and the results from that survey are briefly discussed in our previous paper (McGee and Newton 1982 — Paper I). We now present the experimental details, the 489 observed line profiles and details of the Gaussian analysis of each one. The profiles here are from the ‘main body’ of the SMC. Those of the ‘bridge region’ between the two Clouds of Magellan will form the basis of a later paper.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 4 , Issue 3 , 1982 , pp. 308 - 318
Copyright
Copyright © Astronomical Society of Australia 1982

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References

McGee, R.X., and Newton, Lynette M., Proc. Astron. Soc. Aust., 4, 189 (1982).Google Scholar