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GALEV evolutionary synthesis on the web – current state and future plans

Published online by Cambridge University Press:  13 April 2010

Ralf Kotulla ,
Peter Anders ,
Peter Weilbacher  and
Uta Fritze
Ralf Kotulla
Affiliation:
Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Herts AL10 9AB, United Kingdom email: r.kotulla@galev.org, u.fritze@herts.ac.uk
Peter Anders
Affiliation:
Sterrekundig Instituut, Princetonplein 5, 3584 CC Utrecht, The Netherlands email: p.anders@uu.nl
Peter Weilbacher
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Postdam, Germany email: pweilbacher@aip.de
Uta Fritze
Affiliation:
Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Herts AL10 9AB, United Kingdom email: r.kotulla@galev.org, u.fritze@herts.ac.uk
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Abstract

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GALEV evolutionary synthesis models describe the evolution of stellar populations in general, of star clusters as well as of galaxies, both in terms of resolved stellar populations and of integrated light properties over cosmological timescales of >13 Gyr from the onset of star formation shortly after the Big Bang until today. A new web-interface now allows to run customized GALEV models with user-defined parameters. This web-interface, all data, and many more features to come, can be found at http://www.galev.org.

Keywords

stars: evolution – galaxies: star clusters – galaxies: evolution – methods: numerical
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 366 - 367
Copyright
Copyright © International Astronomical Union 2010

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