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

  • M. R. M. Leão (a1), E. M. de Gouveia Dal Pino (a1), D. Falceta-Gonçalves (a2) (a3), C. Melioli (a1) (a4) and F. G. Geraissate (a1)...

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.

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References

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Falceta-Goncalves, D., Lazarian, A., & Kowal, G. 2008, ApJ 679, 537
Kowal, G. & Lazarian, A. 2007, ApJ 666, L69
Leão, M. R. M., de Gouveia Dal Pino, E. M., Falceta-Gonalves, D., Melioli, C., & Geraissate, F. G., 2008, MNRAS accepted.
Melioli, C., de Gouveia Dal Pino, E. M., & Raga, A. 2005, A&A 443, 495
Melioli, C., de Gouveia Dal Pino, E. M., de la Reza, R., & Raga, A. 2006, MNRAS 373, 811
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Local star formation triggered by SN shocks in magnetized diffuse neutral clouds

  • M. R. M. Leão (a1), E. M. de Gouveia Dal Pino (a1), D. Falceta-Gonçalves (a2) (a3), C. Melioli (a1) (a4) and F. G. Geraissate (a1)...

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