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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

M. R. M. Leão
Affiliation:
Instituto de Astronomia e Geofísica - Universidade de São Paulo, Brazil email: mrmleao@astro.iag.usp.br, dalpino@astro.iag.usp.br
E. M. de Gouveia Dal Pino
Affiliation:
Instituto de Astronomia e Geofísica - Universidade de São Paulo, Brazil email: mrmleao@astro.iag.usp.br, dalpino@astro.iag.usp.br
D. Falceta-Gonçalves
Affiliation:
Núcleo de Astrofísica Teórica, Universidade Cruzeiro do Sul, Brazil Astronomy Department, University of Wisconsin, Madison, USA
C. Melioli
Affiliation:
Instituto de Astronomia e Geofísica - Universidade de São Paulo, Brazil email: mrmleao@astro.iag.usp.br, dalpino@astro.iag.usp.br Dipartimento di Astronomia, Universitá di Bologna, Bologna, Italy
F. G. Geraissate
Affiliation:
Instituto de Astronomia e Geofísica - Universidade de São Paulo, Brazil email: mrmleao@astro.iag.usp.br, dalpino@astro.iag.usp.br
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Abstract

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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
Copyright
Copyright © International Astronomical Union 2009

References

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