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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 ,
E. M. de Gouveia Dal Pino ,
D. Falceta-Gonçalves ,
C. Melioli  and
F. G. Geraissate
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.

Keywords

Stars: star formation – ISM: clouds – Supernova remnants
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

References

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Leão, M. R. M., de Gouveia Dal Pino, E. M., Falceta-Gonalves, D., Melioli, C., & Geraissate, F. G., 2008, MNRAS accepted.Google Scholar
Melioli, C., de Gouveia Dal Pino, E. M., & Raga, A. 2005, A&A 443, 495Google Scholar
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