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Local star formation triggered by SN shocks in magnetized diffuse neutral clouds
Published online by Cambridge University Press: 01 November 2008
Abstract
Considering that the main source of turbulence in the ISM medium are the explosions of supernovae (SNe), we explore here the role of SN shock front interactions with clouds on the star formation triggering in presence and in absence of magnetic field.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Symposium S259: Cosmic Magnetic Fields: From Planets, to Stars and Galaxies , November 2008 , pp. 105 - 106
- Copyright
- Copyright © International Astronomical Union 2009
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