Hostname: page-component-6bf8c574d5-rwnhh Total loading time: 0 Render date: 2025-02-21T17:04:27.518Z Has data issue: false hasContentIssue false
  • English
  • Français

Giant H II Regions in M81

Published online by Cambridge University Press:  04 August 2017

Michele Kaufman ,
R. C. Kennicutt  and
F. N. Bash
Michele Kaufman
Affiliation:
Ohio State University
R. C. Kennicutt
Affiliation:
University of Minnesota
F. N. Bash
Affiliation:
University of Texas

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Giant HII regions are important tracers of recent star formation in distant galaxies. For a selection of HII regions in our galaxy where the exciting stars can be identified, Rumstay (1985) finds that the measured Hα and radio continuum luminosities of an HII region correlate with the stellar ionizing flux derived from model atmospheres and the known exciting stars. Therefore, we use flux measurements of giant HII regions as an index of the distribution of O stars in M81.

Type
Poster Papers 4
Information
Symposium - International Astronomical Union , Volume 116: Luminous Stars and Associations in Galaxies , 1986 , pp. 503 - 504
Copyright
Copyright © Reidel 1986 

References

Bash, F.N., and Kaufman, M. 1985, Bull. A.A.S., 16, 976.Google Scholar
Connolly, L.P., Mantarakis, P.Z., and Thompson, L.A. 1972, Publ. A.S.P. 84, 61.CrossRefGoogle Scholar
Hodge, P.W., and Kennicutt, R.C. 1983, Astron. J. 88, 296.CrossRefGoogle Scholar
Leisawitz, D., and Bash, F. 1982, Astrophys. J. 259, 133.CrossRefGoogle Scholar
Rumstay, K.S. 1985, preprint.Google Scholar
Rumstay, K.S., and Kaufman, M. 1983, Astrophys. J. 274, 611.CrossRefGoogle Scholar
Visser, H.C.D. 1980, Astron. Astrophys. 88, 159.Google Scholar