Local star formation triggered by SN shocks in magnetized diffuse neutral clouds

Details Local star formation triggered by SN shocks in magnetized diffuse neutral clouds Local star formation triggered by SN shocks in magnetized diffuse neutral clouds

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009iaus..259..105l&link_type=abstract

Cosmic Magnetic Fields: From Planets, to Stars and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium,

Astronomy and Astrophysics

Astronomy

Stars: Star Formation, Ism: Clouds, Supernova Remnants

Scientific paper

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.

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