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

M. R. M. Leao; E. M. de Gouveia Dal Pino; D. Falceta-Goncalves; C. Melioli; F. G. Geraissate

doi:10.1017/S1743921309030191

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

M. R. M. Leao^*, E. M. de Gouveia Dal Pino, D. Falceta-Goncalves, C. Melioli, F. G. Geraissate

^*Corresponding author for this work

School of Physics and Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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.

Original language	English
Title of host publication	COSMIC MAGNETIC FIELDS: FROM PLANETS, TO STARS AND GALAXIES
Editors	KG Strassmeier, AG Kosovichev, JE Beckman
Place of Publication	CAMBRIDGE
Publisher	Cambridge University Press
Pages	105-106
Number of pages	2
ISBN (Print)	978-0-521-88990-2
DOIs	https://doi.org/10.1017/S1743921309030191
Publication status	Published - 2009
Event	259th Symposium of the International-Astronomical-Union - Puerto Santiago, Spain Duration: 3 Nov 2008 → 7 Nov 2008

Publication series

Name	IAU Symposium Proceedings Series
Publisher	CAMBRIDGE UNIV PRESS
Volume	4
ISSN (Print)	1743-9213

Conference

Conference	259th Symposium of the International-Astronomical-Union
Country/Territory	Spain
City	Puerto Santiago
Period	3/11/08 → 7/11/08

Keywords

Stars: star formation
ISM: clouds
Supernova remnants

Access to Document

10.1017/S1743921309030191

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Leao, M. R. M., de Gouveia Dal Pino, E. M., Falceta-Goncalves, D., Melioli, C., & Geraissate, F. G. (2009). Local star formation triggered by SN shocks in magnetized diffuse neutral clouds. In KG. Strassmeier, AG. Kosovichev, & JE. Beckman (Eds.), COSMIC MAGNETIC FIELDS: FROM PLANETS, TO STARS AND GALAXIES (pp. 105-106). (IAU Symposium Proceedings Series; Vol. 4). Cambridge University Press. https://doi.org/10.1017/S1743921309030191

@inproceedings{0d32de922d794c2aac743bebd5f8cff5,

title = "Local star formation triggered by SN shocks in magnetized diffuse neutral clouds",

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.",

keywords = "Stars: star formation, ISM: clouds, Supernova remnants",

author = "Leao, {M. R. M.} and {de Gouveia Dal Pino}, {E. M.} and D. Falceta-Goncalves and C. Melioli and Geraissate, {F. G.}",

year = "2009",

doi = "10.1017/S1743921309030191",

language = "English",

isbn = "978-0-521-88990-2",

series = "IAU Symposium Proceedings Series",

publisher = "Cambridge University Press",

pages = "105--106",

editor = "KG Strassmeier and AG Kosovichev and JE Beckman",

booktitle = "COSMIC MAGNETIC FIELDS: FROM PLANETS, TO STARS AND GALAXIES",

address = "United Kingdom",

note = "259th Symposium of the International-Astronomical-Union ; Conference date: 03-11-2008 Through 07-11-2008",

}

Leao, MRM, de Gouveia Dal Pino, EM, Falceta-Goncalves, D, Melioli, C & Geraissate, FG 2009, Local star formation triggered by SN shocks in magnetized diffuse neutral clouds. in KG Strassmeier, AG Kosovichev & JE Beckman (eds), COSMIC MAGNETIC FIELDS: FROM PLANETS, TO STARS AND GALAXIES. IAU Symposium Proceedings Series, vol. 4, Cambridge University Press, CAMBRIDGE, pp. 105-106, 259th Symposium of the International-Astronomical-Union, Puerto Santiago, Spain, 3/11/08. https://doi.org/10.1017/S1743921309030191

Local star formation triggered by SN shocks in magnetized diffuse neutral clouds. / Leao, M. R. M.; de Gouveia Dal Pino, E. M.; Falceta-Goncalves, D. et al.
COSMIC MAGNETIC FIELDS: FROM PLANETS, TO STARS AND GALAXIES. ed. / KG Strassmeier; AG Kosovichev; JE Beckman. CAMBRIDGE: Cambridge University Press, 2009. p. 105-106 (IAU Symposium Proceedings Series; Vol. 4).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - Local star formation triggered by SN shocks in magnetized diffuse neutral clouds

AU - Leao, M. R. M.

AU - de Gouveia Dal Pino, E. M.

AU - Falceta-Goncalves, D.

AU - Melioli, C.

AU - Geraissate, F. G.

PY - 2009

Y1 - 2009

N2 - 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.

AB - 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.

KW - Stars: star formation

KW - ISM: clouds

KW - Supernova remnants

U2 - 10.1017/S1743921309030191

DO - 10.1017/S1743921309030191

M3 - Conference contribution

SN - 978-0-521-88990-2

T3 - IAU Symposium Proceedings Series

SP - 105

EP - 106

BT - COSMIC MAGNETIC FIELDS: FROM PLANETS, TO STARS AND GALAXIES

A2 - Strassmeier, KG

A2 - Kosovichev, AG

A2 - Beckman, JE

PB - Cambridge University Press

CY - CAMBRIDGE

T2 - 259th Symposium of the International-Astronomical-Union

Y2 - 3 November 2008 through 7 November 2008

ER -

Leao MRM, de Gouveia Dal Pino EM, Falceta-Goncalves D, Melioli C, Geraissate FG. Local star formation triggered by SN shocks in magnetized diffuse neutral clouds. In Strassmeier KG, Kosovichev AG, Beckman JE, editors, COSMIC MAGNETIC FIELDS: FROM PLANETS, TO STARS AND GALAXIES. CAMBRIDGE: Cambridge University Press. 2009. p. 105-106. (IAU Symposium Proceedings Series). doi: 10.1017/S1743921309030191

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

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