Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-18T05:25:43.236Z Has data issue: false hasContentIssue false

HI in the Small Magellanic Cloud Re-examined — II

Published online by Cambridge University Press:  25 April 2016

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

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
Copyright
Copyright © Astronomical Society of Australia 1982

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

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