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Multiwavelength Mapping of Galaxy Formation and Evolution pp 361–362Cite as

Beyond the Lick Indices: The High-Resolution Spectral Synthesis of Stellar Populations

Part of the ESO Astrophysics Symposia book series (ESO)

Abstract

Up-to-date theoretical SED of stellar populations at 2 Å FWHM resolution is obtained by coupling a new library of synthetic spectra from the ATLAS and NextGen atmosphere database with the Buzzoni population synthesis code. We briefly outline the current status of the project, aimed at settling a new theoretical framework of narrow-band spectrophotometric indices to study stellar populations of galaxies.

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Authors and Affiliations

  1. INAF – Osservatorio Astronomico di Bologna, Italy

    Alberto Buzzoni

  2. INAF – Osservatorio Astronomico di Brera-Milano, Italy

    Alberto Buzzoni

  3. INAOE – Instituto Nacional de Astrofisica, Optica y Electronica, Puebla, Mexico

    Emanuele Bertone, Lino H. Rodríguez-Merino & Miguel Chávez

Authors
  1. Alberto Buzzoni
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  2. Emanuele Bertone
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  3. Lino H. Rodríguez-Merino
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  4. Miguel Chávez
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Editor information

Alvio Renzini Ralf Bender

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Cite this paper

Buzzoni, A., Bertone, E., Rodríguez-Merino, L.H., Chávez, M. Beyond the Lick Indices: The High-Resolution Spectral Synthesis of Stellar Populations. In: Renzini, A., Bender, R. (eds) Multiwavelength Mapping of Galaxy Formation and Evolution. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10995020_61

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  • DOI: https://doi.org/10.1007/10995020_61

  • Published:

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-25665-6

  • Online ISBN: 978-3-540-31641-1

  • eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)

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