Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-22T15:00:36.588Z Has data issue: false hasContentIssue false
  • English
  • Français

Young and old massive star clusters and their stellar populations - Theoretical challenges for the next decade

Published online by Cambridge University Press:  31 March 2017

Corinne Charbonnel
Corinne Charbonnel*
Affiliation:
Department of Astronomy, University of Geneva, 1290 Versoix - Switzerland email: [email protected] IRAP CNRS UMR 5277, Université de Toulouse III, 31400 Toulouse, France
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.

Several models presented in the literature compete to explain the origin of multiple stellar populations in globular clusters (GC), but they all fail to reproduce the large variety of present-day characteristics of these systems. In parallel, independent clues on GC early evolution may be derived from observations of young massive clusters (YMC) in the Local Group. But are these two populations of clusters related? And can we reconcile the informations and data concerning GCs and YMCs? Here we summarize some open questions on the nucleosynthetic origin of multiple stellar populations in GCs, on the actual evolution and characteristics of GC low-mass stars, and on early gas expulsion from massive clusters. We propose theoretical paths to be explored in the near future.

Keywords

globular clusters: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S316: Formation, evolution, and survival of massive star clusters , August 2015 , pp. 1 - 8
Copyright
Copyright © International Astronomical Union 2017 

References

Bastian, N., et al., 2013, MNRAS, 436, 2398 Google Scholar
Bastian, N., Hollyhead, K, & Cabrera-Ziri, I., 2014, MNRAS, 445, 378 Google Scholar
Bastian, N., Cabrera-Ziri, I., & Salaris, M., 2015, MNRAS, 445, 378 Google Scholar
Bastian, N., & Lardo, C., 2015, MNRAS, 449, 3333 Google Scholar
Bragaglia, A., et al. 2014, ApJ, 796, 68 Google Scholar
Campbell, S. W., et al. 2013, Nature, 498, 198 Google Scholar
Carretta, E., et al. 2009, A&A 505, 139 Google Scholar
Carretta, E., et al. 2010, A&A, 516, A55 Google Scholar
Carretta, E. 2010, A&A, 557, A128 Google Scholar
Cassisi, S., Mucciarelli, A., Pientriferni, A., Salaris, M., & Ferduson, J. 2013, A&A, 554, A19 Google Scholar
Chantereau, W., Charbonnel, C., & Decressin, T. 2015, A&A, 578, A117 Google Scholar
Chantereau, W., Charbonnel, C., & Meynet, G. 2016, submitted to A&A Google Scholar
Charbonnel, C. & Krause, M., 2015, IAUS 317 “The General Assembly of the Galactic Halo”, in pressGoogle Scholar
Charbonnel, C. & Lagarde, N. 2010, A&A, 522, A10 Google Scholar
Charbonnel, C. & Zahn, J. P. 2007, A&A (Letter), 467, L15 Google Scholar
Charbonnel, C., et al. 2013, A&A (Letter), 557, L17 Google Scholar
Charbonnel, C., Chantereau, W., Krause, M., Primas, F., & Wang, Y. 2014, A&A (Letter), 569, L6 (C14)Google Scholar
Charbonnel, C., & Chantereau, W., 2015, A&A, in pressGoogle Scholar
Chiappini, C. 2008, A&A, 479, L9 Google Scholar
D'Antona, F. & Caloi, V. 2004, ApJ, 611, 871 Google Scholar
D'Antona, F., et al. 2012, A&A, 443, 3302 Google Scholar
Decressin, T., et al. 2007a, A&A, 464, 1029 Google Scholar
Decressin, T., Charbonnel, C. & Meynet, G. 2007b, A&A, 475, 859 Google Scholar
Decressin, T., Charbonnel, C., et al. 2009, A&A, 505, 727 Google Scholar
Decressin, T., Baumgardt, H., Charbonnel, C., & Kroupa, P., 2010, A&A, 516, A73 Google Scholar
De Mink, S., et al. 2009, A&A (Letters), 507, L1 Google Scholar
Denissenkov, P. A. & Herwig, F. 2003, ApJ, 590, L99 CrossRefGoogle Scholar
Denissenkov, P. A. & Hartwick, F. D. A. 2014, MNRAS (Letter), 437, L21 Google Scholar
D'Ercole, , et al. 2010, MNRAS, 407, 854 Google Scholar
D'Ercole, , et al. 2010, MNRAS, 423, 1521 Google Scholar
Doherty, C. L., et al. 2014, MNRAS, 437, 195 CrossRefGoogle Scholar
Dotter, , et al. 2010, ApJ, 708, 698 CrossRefGoogle Scholar
Forestini, M. & Charbonnel, C. 1997, A&A, 123, 241 Google Scholar
Gratton, R. G., et al. 2010, A&A, 517, A81 Google Scholar
Karakas, A. & Lattanzio, J. 2007, PASA 24, 103 CrossRefGoogle Scholar
Khalaj, P. & Baumgardt, H. 2015, MNRAS, 492, 924 Google Scholar
Gratton, R. G., Carretta, E., & Bragaglia, A. 2012, ARAA, 20, 50 Google Scholar
Krause, M., Charbonnel, C., et al. 2012, A&A (Letter), 546, L5 Google Scholar
Krause, M., Charbonnel, C., et al. 2013, A&A, 552, A121 Google Scholar
Krause, M., Charbonnel, C., Bastian, N., & Diehl, R. 2016, A&A, in press, arXiv:1512.04256 (K15)Google Scholar
Kroupa, P., et al. 2013, in Planets, Stars and Stellar Systems (Springer Netherlands), 115 Google Scholar
Lagarde, N., et al. 2012, A&A, 543, A108 Google Scholar
Larsen, S. S., et al. 2014, A&A, 565, A98 Google Scholar
Lind, K., et al. 2009, A&A, 503, 545 Google Scholar
Maeder, A. & Meynet, G. 2006, A&A, 448, L37 Google Scholar
Marino, A. F., et al. 2014, MNRAS, 437, 1609 Google Scholar
Marino, A. F., et al. 2015, MNRAS, 450, 815 Google Scholar
Martell, S. L., Molinski, J. P., Beers, T. C., & Grebel, E. K. 2011, A&A, 354, A136 Google Scholar
Milone, A. P., Marino, A. F., Piotto, G. P., et al. 2013, ApJ, 767, 120 Google Scholar
Milone, A. P., Marino, A. F., Piotto, G. P., et al. 2015, ApJ, 808, 51 Google Scholar
Piotto, G., et al. 2002, ApJ, 670, 39 Google Scholar
Prantzos, N. & Charbonnel, C. 2006, A&A, 458, 135 Google Scholar
Prantzos, N., Charbonnel, C., & Iliadis, C. 2007, A&A, 470, 179 Google Scholar
Renzini, A., et al. 2015, MNRAS, 454, 4197 Google Scholar
Sbordone, L., Salaris, M., Weiss, A., & Cassisi, S. 2011, A&A, 534, A9 Google Scholar
Schaerer, D. & Charbonnel, C. 2011, MNRAS, 413, 2297 Google Scholar
Sills, A. & Glebbeek, E. 2010, MNRAS 407, 277 Google Scholar
Simmerer, J., et al. 2013, ApJ (Letters), 764, L7 Google Scholar
Smith, G. H. & Norris, J. 1982, ApJ, 254, 594 Google Scholar
Ventura, P., et al. 2001, ApJ (Letter), 550, L65 Google Scholar
Ventura, P., et al. 2013, MNRAS, 431, 3642 Google Scholar