Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-10T22:33:48.451Z Has data issue: false hasContentIssue false
  • English
  • Français

BaSTI – a library of stellar evolution models: updates and applications

Published online by Cambridge University Press:  01 December 2006

A. Pietrinferni ,
S. Cassisi ,
M. Salaris ,
D. Cordier  and
F. Castelli
A. Pietrinferni
Affiliation:
INAF – Astronomical Observatory of Collurania, via M. Maggini 64100 Teramo, Italy email: pietrinferni@oa-teramo.inaf.it, cassisi@oa-teramo.inaf.it
S. Cassisi
Affiliation:
INAF – Astronomical Observatory of Collurania, via M. Maggini 64100 Teramo, Italy email: pietrinferni@oa-teramo.inaf.it, cassisi@oa-teramo.inaf.it
M. Salaris
Affiliation:
Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Birkenhead, CH41 1LD, UK email: ms@astro.livjm.ac.uk
D. Cordier
Affiliation:
Ecole Nationale Superieure de Chimie de Rennes, Campus de Beaulieu, 35700 Rennes, France, email: daniel.cordier@ensrc-rennes.fr
F. Castelli
Affiliation:
INAF – Astronomical Observatory of Trieste, via Tiepolo 11, 34131 Trieste, Italy, email: castelli@ts.astro.it
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.

We present a new library of stellar evolution models for a large range of masses and chemical compositions, based on an up-to-date theoretical framework. We briefly discuss the physical inputs and the assumptions adopted in computing the models. The last developments of this database are also presented.

Keywords

stars: evolutionstars: pre-main-sequence stars: luminosity function
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 39 - 40
Copyright
Copyright © International Astronomical Union 2007

References

Alexander,, D.R., & Ferguson, J. W. 1994, ApJ 437, 879CrossRefGoogle Scholar
Angulo, C. et al. (NACRE coll.) 1999, Nuclear Physics A 656, 3CrossRefGoogle Scholar
Ferguson, J. W. et al. 2005, ApJ 623, 585CrossRefGoogle Scholar
Grevesse, N. & Noels, A. 1993, in: Prantzos, N., Vangioni-Flam, E., Casse, M. (eds.), Origin and Evolution of the Elements, (Cambridge University Press), 15Google Scholar
Kunz, R. et al. 2002, ApJ 567, 643CrossRefGoogle Scholar
Iglesias, C. A., & Rogers, F. J. 1996, ApJ 464, 943CrossRefGoogle Scholar
Pietrinferni, A. et al. 2004, ApJ 612, 168CrossRefGoogle Scholar
Pietrinferni, A. et al. 2006, ApJ 642, 797CrossRefGoogle Scholar
Potekhin, A. Y. 1999, A&A 351, 787Google Scholar
Weiss, A. et al. 2006, astro-ph/0605666Google Scholar