The SAURON project – XVII. Stellar population analysis of the absorption line strength maps of 48 early-type galaxies

@article{Kuntschner2010TheSP,
  title={The SAURON project – XVII. Stellar population analysis of the absorption line strength maps of 48 early-type galaxies},
  author={Harald Kuntschner and Eric Emsellem and Roland Bacon and Michele Cappellari and Roger Davies and P. T. de Zeeuw and Jes'us Falc'on-Barroso and Davor Krajnovi'c and Richard M. McDermid and Reynier F. Peletier and Marc Sarzi and Kristen Leah Shapiro and Remco van den Bosch and Glenn van de Ven},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2010},
  volume={408},
  pages={97-132}
}
We present a stellar population analysis of the absorption line strength maps for 48 early-type galaxies from the SAURON sample. Using the line strength index maps of H beta, Fe5015 and Mgb, measured in the Lick/IDS system and spatially binned to a constant signal-to-noise ratio, together with predictions from up-to-date stellar population models, we estimate the simple stellar population-equivalent (SSP-equivalent) age, metallicity and abundance ratio [alpha/Fe] over a two-dimensional field… Expand
ATLAS3D Stellar Population Gradients
  • H. Kuntschner
  • Physics
  • Proceedings of the International Astronomical Union
  • 2014
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