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Element abundance ratios in stellar population modelling

Published online by Cambridge University Press:  27 October 2016

Daniel Thomas
Daniel Thomas*
Affiliation:
Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Burnaby Road, Portsmouth, PO1 3FX, UK. email: daniel.thomas@port.ac.ukSEPnet, South East Physics Network, (www.sepnet.ac.uk)
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Abstract

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I review the implementation of the effects from varying chemical element abundance ratios in stellar population modelling. Recent highlights include the adoption of new flux calibrated libraries, the inclusion of a wide range of chemical elements, the calculation of error estimates on the model, and the consideration of element variation effects on full spectra. Some key results on the element ratios measured in early-type galaxies are discussed.

Keywords

stars: abundances - galaxies: abundances - galaxies: stellar content
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 188 - 189
Copyright
Copyright © International Astronomical Union 2016 

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