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.
No takes yet. Share an insight, caveat, or question.
McGee et al. (1982) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: