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Strongly triggered collapse model confronts observations

Published online by Cambridge University Press:  01 August 2006

Patrick Hennebelle ,
Arnaud Belloche ,
Philippe André  and
Anthony Whitworth
Patrick Hennebelle
Affiliation:
Laboratoire de Radioastronomie Millimétrique, UMR 8112 du CNRS, École Normale Supérieure et Observatoire de Paris, 24 rue Lhomond 75231 Paris Cedex 05Francepatrick.hennebelle@ens.fr
Arnaud Belloche
Affiliation:
Max Planck-Institut fur Radioastronomie, Auf dem Hugel 69, 53121 Bonn, Germany email: belloche@mpifr-bonn.mpg.de
Philippe André
Affiliation:
Service d'Astrophysique, CEA/DSM/DAPNIA, C.E. Saclay, 91191 Gif-sur-Yvette Cedex, France email: pandre@cea.fr
Anthony Whitworth
Affiliation:
School of Physics & Astronomy, Cardiff University, 5 The Parade, Cardiff CF24 3YB, Wales, UK email: ant@astro.cf.ac.uk
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Abstract

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Detailed modelling of individual protostellar condensations is important to test the various theories. Here we present comparisons between strongly induced collapse models with one young class-0 object, IRAS4A, in the Perseus cloud and one prestellar cloud observed in the Coalsack molecular cloud.

Keywords

stars:formationhydrodynamicsgravitation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 265 - 269
Copyright
Copyright © International Astronomical Union 2007

References

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