Element abundance ratios in stellar population modelling
Research output: Contribution to journal › Review article › peer-review
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.
|Number of pages||2|
|Journal||Proceedings of the International Astronomical Union|
|Publication status||Published - 27 Oct 2016|
|Event||XXIXth IAU General Assembly - Honolulu, United States|
Duration: 3 Aug 2015 → 14 Aug 2015