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How did globular clusters lose their gas?

Published online by Cambridge University Press:  05 March 2015

C. Charbonnel ,
M. Krause ,
T. Decressin ,
G. Meynet ,
N. Prantzos  and
R. Diehl
C. Charbonnel
Affiliation:
Geneva Observatory, University of Geneva, Versoix, Swizerland IRAP, CNRS UMR 5277, Toulouse, France
M. Krause
Affiliation:
Geneva Observatory, University of Geneva, Versoix, Swizerland Excellence Cluster Universe, Technische Universität München, Garching, Germany Max-Planck-Institut für extraterrestrische Physik, Garching, Germany
T. Decressin
Affiliation:
Geneva Observatory, University of Geneva, Versoix, Swizerland
G. Meynet
Affiliation:
Geneva Observatory, University of Geneva, Versoix, Swizerland
N. Prantzos
Affiliation:
Institut d'Astrophysique de Paris, CNRS UMR7095, Paris, France
R. Diehl
Affiliation:
Excellence Cluster Universe, Technische Universität München, Garching, Germany Max-Planck-Institut für extraterrestrische Physik, Garching, Germany
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Abstract

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We summarize the results presented in Krause et al. (2012a, K12) on the impact of supernova-driven shells and dark-remnant accretion on gas expulsion in globular cluster infancy.

Keywords

Globular clusters - ISM: bubbles
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 255 - 256
Copyright
Copyright © International Astronomical Union 2015 

References

Decressin, T., Charbonnel, C., & Meynet, G., 2007, A&A 475, 859Google Scholar
Decressin, T., Baumgardt, H., Charbonnel, C., & Kroupa, P., 2010, A&A 516, A73Google Scholar
D'Ercole, A., Vesperini, E., D'Antona, F., et al., 2008, MNRAS 391, 825CrossRefGoogle Scholar
Krause, M., Charbonnel, C., Decressin, T., Meynet, G., Prantzos, N., & Diehl, R., 2012a, A&A 546, L5 (K12)Google Scholar
Schaerer, D., & Charbonnel, C., 2011, MNRAS 413, 2297Google Scholar
Vesperini, E., McMillan, S. L. W., D'Antona, F., & D'Ercole, A., 2010, ApJ 718, L112Google Scholar