Astrophysics and Space Science

, Volume 78, Issue 2, pp 273–285

Sequential explosions of supernovae in an ob association and formation of a superbubble

Authors

  • Kohji Tomisaka
    • Department of PhysicsHokkaido University
  • Asao Habe
    • Department of PhysicsHokkaido University
  • Satoru Ikeuchi
    • Department of PhysicsHokkaido University
Article

DOI: 10.1007/BF00648941

Cite this article as:
Tomisaka, K., Habe, A. & Ikeuchi, S. Astrophys Space Sci (1981) 78: 273. doi:10.1007/BF00648941

Abstract

From the standpoint of view that the early type stars are formed sequentially at an OB association, it is expected that the supernova explosions will also occur sequentially. We study the expansion law of a supernova remnant, which is formed by sequential explosions of supernovae. The superbubbles and supershells with the radii 200∼1000 pc are naturally explained by this model. Assuming that the sequential explosion of supernovae occurs at every OB association, we deduce the star formation rate in our Galaxy.

Copyright information

© D. Reidel Publishing Co 1981