Hostname: page-component-8448b6f56d-xtgtn Total loading time: 0 Render date: 2024-04-25T04:06:14.941Z Has data issue: false hasContentIssue false
  • English
  • Français

Physics and modes of star cluster formation

Published online by Cambridge University Press:  18 January 2010

Matthew R. Bate
Matthew R. Bate*
Affiliation:
School of Physics, University of Exeter, Stocker Road, Exeter EX4 4QL, UK email: mbate@astro.ex.ac.uk
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

I review the progress made in understanding the physics and modes of star cluster formation through the use of direct self-gravitating hydrodynamical simulations, including those that have recently been performed incorporating radiative transfer and magnetic fields.

Keywords

gravitationhydrodynamicsMHDradiative transferstellar dynamicsmethods: numericalstars: formationstars: low-massbrown dwarfsstars: luminosity functionmass function
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S266: Star clusters: basic galactic building blocks throughout time and space , August 2009 , pp. 29 - 34
Copyright
Copyright © International Astronomical Union 2010

References

Bate, M. R. 2005, MNRAS, 363, 363CrossRefGoogle Scholar
Bate, M. R. 2009a, MNRAS, 392, 590Google Scholar
Bate, M. R. 2009b, MNRAS, 392, 1363CrossRefGoogle Scholar
Bate, M. R. 2009c, MNRAS, 397, 232Google Scholar
Bate, M. R. & Bonnell, I. A. 2005, MNRAS, 356, 1201CrossRefGoogle Scholar
Bate, M. R., Bonnell, I. A., & Bromm, V. 2002a, MNRAS (Letters), 332, L65CrossRefGoogle Scholar
Bate, M. R., Bonnell, I. A., & Bromm, V. 2002b, MNRAS, 336, 705CrossRefGoogle Scholar
Bate, M. R., Bonnell, I. A., & Bromm, V. 2003, MNRAS, 339, 577Google Scholar
Bonnell, I. A., Bate, M. R., Clarke, C. J., & Pringle, J. E. 1997, MNRAS, 285, 201Google Scholar
Bonnell, I. A., Bate, M. R., & Vine, S. G. 2003, MNRAS, 343, 413CrossRefGoogle Scholar
Bonnell, I. A., Clarke, C. J., & Bate, M. R. 2006, MNRAS, 368, 1296Google Scholar
Brunt, C. M., Heyer, M. H., & Mac Low, M.-M. 2009, MNRAS, 504, 883Google Scholar
Evans, N. J., et al. 2009, ApJS, 181, 321CrossRefGoogle Scholar
Goldsmith, P. F., Heyer, M., Narayanan, G., Snell, R., Li, D., & Brunt, C. 2008, ApJ, 680, 428Google Scholar
Hennebelle, P. & Fromang, S. 2008, A&A, 477, 9Google Scholar
Hennebelle, P. & Teyssier, R. 2008, A&A, 477, 25Google Scholar
Jappsen, A.-K., Klessen, R. S., Larson, R. B., Li, Y., & Mac Low, M.-M. 2005, A&A, 435, 611Google Scholar
Klessen, R. S. 2001, ApJ, 550, 77CrossRefGoogle Scholar
Klessen, R. S. & Burkert, A. 2000, ApJS, 128, 287CrossRefGoogle Scholar
Klessen, R. S. & Burkert, A. 2001b, ApJ, 549, 386CrossRefGoogle Scholar
Klessen, R. S., Burkert, A., & Bate, M. R. 1998, ApJ (Letters), 501, L205Google Scholar
Krumholz, M. R., McKee, C. F., & Klein, R.I. 2004, ApJ, 611, 399CrossRefGoogle Scholar
Larson, R. B. 1981, MNRAS, 194, 809CrossRefGoogle Scholar
Offner, S. S. R., Klein, R. I., & McKee, C. F. 2008, ApJ, 686, 1174CrossRefGoogle Scholar
Offner, S. S. R., Klein, R. I., McKee, C. F., & Krumholz, M. R. 2009, ApJ, 703, 131Google Scholar
Price, D. J. & Bate, M. R. 2007, MNRAS, 377, 77CrossRefGoogle Scholar
Price, D. J. & Bate, M. R. 2008, MNRAS, 385, 1820CrossRefGoogle Scholar
Price, D. J. & Bate, M. R. 2009, MNRAS, 398, 33CrossRefGoogle Scholar