Abstract
The H ∞ tregions of the Large Magellanic Cloud with diameters D ≧25″≊ -6 pc delineate a clear spiral pattern corresponding to a ScIII-IVp galaxy. The supergiant HII complex 30 Doradus appears to be the mildly active nucleus of the LMC.
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References
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Feitzinger, J., Schmidt-Kaler, Th. 1975, Astr. and Ap. submitted.
Isserstedt, J., Schmidt-Kaler, Th. 1975, Astr. and Ap. in press.
Mathewson, D.S., Healey, J.R. 1964, I.A.U. Symp. No. 20: The Galaxy and the Magellanic Clouds, ed. F.J. Kerr and A.W. Rodgers (Canberra: Australian Academy of Science), p. 245.
Schmidt-Kaler, Th., Isserstedt, J. 1975, Astr. and Ap. submitted.
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Schmidt-Kaler, T. (1975). The distribution of HII regions in the large magellanic cloud. In: Wilson, T.L., Downes, D. (eds) H II Regions and Related Topics. Lecture Notes in Physics, vol 42. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-07409-0_141
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DOI: https://doi.org/10.1007/3-540-07409-0_141
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