The Messier 82 Starburst Galaxy

  • A. Pedlar
  • K.A. Wills
Part of the Astrophysics and Space Science Proceedings book series (ASSSP)


All galaxies show some degree of star formation, although the star formation rate differs greatly between different classes of galaxies. Early types, such as ellipticals, clearly show significantly less star formation than late types, such as spirals and irregulars. Much of the current star formation in spiral galaxies is associated with spiral arms, and appears to be due to the interaction of stellar density waves which drive shocks into neutral gas.


Star Formation Supernova Remnant Star Formation Rate Neutral Hydrogen Compact Source 
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 2007

Authors and Affiliations

  • A. Pedlar
    • 1
  • K.A. Wills
    • 2
  1. 1.JBO, University of ManchesterCheshire
  2. 2.Department of Physics & AstronomyUniversity of ShefieldSheffield

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