GALEV evolutionary synthesis models - I. Code, input physics and web-interface
Ralf Kotulla, Uta Fritze, Peter Weilbacher, Peter Anders

TL;DR
GALEV models simulate stellar population evolution in galaxies and star clusters, incorporating chemical and spectral evolution over cosmological timescales, and are now accessible via an interactive web interface for diverse astrophysical applications.
Contribution
The paper introduces the latest version of GALEV models with an interactive web interface, detailing input physics and enabling customizable simulations for various astrophysical objects.
Findings
Models cover a wide range of metallicities and galaxy types.
Chemical evolution is integrated with spectral evolution.
Models are accessible online for research use.
Abstract
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. For galaxies, GALEV includes a simultaneous treatment of the chemical evolution of the gas and the spectral evolution of the stellar content, allowing for what we call a chemically consistent treatment: We use input physics (stellar evolutionary tracks, stellar yields and model atmospheres) for a large range of metallicities and consistently account for the increasing initial abundances of successive stellar generations. Here we present the latest version of the galev evolutionary synthesis models that are now interactively available at www.galev.org. We…
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