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H II Regions and Supernova Remnants

  • Paul Hodge
Part of the Astrophysics and Space Science Library book series (ASSL, volume 176)

Abstract

There has been relatively little research done so far on the H II regions of M31, beyond the task of identifying them and cataloging the brightest several hundred. At the time of this writing, however, at least two groups of scientists are working on detailed studies of the H II regions and so this chapter is likely to be outdated to some extent rather soon. For supernova remnants, on the other hand, more has been completed, especially at radio wavelengths.

Keywords

Rotation Curve Emission Region Supernova Remnant Luminosity Function Nearby Galaxy 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media Dordrecht 1992

Authors and Affiliations

  • Paul Hodge
    • 1
  1. 1.Department of AstronomyUniversity of WashingtonSeattleUSA

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