Hostname: page-component-6bf8c574d5-gr6zb Total loading time: 0 Render date: 2025-02-21T16:53:19.667Z Has data issue: false hasContentIssue false
  • English
  • Français

The Dynamical Evolution of Expanding HI Shells and Initial Mass Function of OB Associations

Published online by Cambridge University Press:  04 August 2017

S.A. Silich
S.A. Silich*
Affiliation:
Main Astronomical Observatory Academy of Sciences of the Ukrainian SSR 252127 Kiev-127, Goloseevo USSR

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 evolution of expanding supershells produced by SN explosion in OB associations is considered. The expansion velocities of the shells and OB associations IMF spectral index are obtained. The results agree well with observational data.

Type
Poster Papers 3
Information
Symposium - International Astronomical Union , Volume 116: Luminous Stars and Associations in Galaxies , 1986 , pp. 393 - 394
Copyright
Copyright © Reidel 1986 

References

Tomisaka, K., Habe, A., Ikeuchi, S.: 1981, Astrophys. Spase Sci., 78, 273.CrossRefGoogle Scholar
Heiles, C.: 1979, Astrophys. J., 229, 533.CrossRefGoogle Scholar
Elmegreen, B.G., Elmegreen, D.M.: 1988, MNRAS, 203, 31.Google Scholar
Bisincehi, G.F., Fermani, G., Sarmiento, A.F.: 1983, Astron. Astrophys., 119, 167.Google Scholar
Bruhweiler, F.G., Gull, T.R., Kafatos, M., Sofia, S.: 1980, Astrophys. J., 238, L27.Google Scholar