Hostname: page-component-76fb5796d-vfjqv Total loading time: 0 Render date: 2024-04-26T08:06:48.523Z Has data issue: false hasContentIssue false
  • English
  • Français

The Hiiregions of M31

Published online by Cambridge University Press:  14 August 2015

J. H. Spencer  and
B. F. Burke
J. H. Spencer
Affiliation:
Dept. of Physics and Research Laboratory of Electronics, Massachusetts Institute of Technology, Cambridge, Mass., U.S.A.
B. F. Burke
Affiliation:
Dept. of Physics and Research Laboratory of Electronics, Massachusetts Institute of Technology, Cambridge, Mass., U.S.A.

Abstract

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.

The luminosity of the brightest Hiiregions of M31 was determined with the NRAO 3-element interferometer at 3.7 cm and 11 cm wavelength. It is unlikely that M31 has any superbright Hiiregions such as W51 or W49; our Galaxy has between 10 and 20 Hiiregions that are more luminous than any in M31.

Type
Part 2: Galactic H ii Regions
Information
Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 229 - 231
Copyright
Copyright © Reidel 1974 

References

Baade, W. and Arp, H. C.: 1964, Astrophys. J. 139, 1027.Google Scholar
Reifenstein, E. C. III, Wilson, T. L., Burke, B. F., Mezger, P. G., and Altenhoff, W. J.: 1970, Astron. Astrophys. 4, 357.Google Scholar
Wilson, T. L., Mezger, P. G., Gardner, F. F., and Milne, D. K.: 1970, Astron. Astrophys. 6, 364.Google Scholar