Advertisement

The distribution of HII regions in the large magellanic cloud

  • TH. Schmidt-Kaler
Part VII: H II Regions Associated with Nuclei of Galaxies
Part of the Lecture Notes in Physics book series (LNP, volume 42)

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.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. Broten, N.W. 1972, Austral. J. Phys. 25, 599Google Scholar
  2. Feitzinger, J., Schmidt-Kaler, Th. 1975, Astr. and Ap. submitted.Google Scholar
  3. Isserstedt, J., Schmidt-Kaler, Th. 1975, Astr. and Ap. in press.Google Scholar
  4. 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.Google Scholar
  5. Schmidt-Kaler, Th., Isserstedt, J. 1975, Astr. and Ap. submitted.Google Scholar

Copyright information

© Springer-Verlag 1975

Authors and Affiliations

  • TH. Schmidt-Kaler
    • 1
  1. 1.Astronomisches Institut der UniversitätBochumGermany

Personalised recommendations