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Photometric and Spectrophotometric Models in the NIR

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Part of the book series: ESO Astrophysics Symposia ((ESO))

Abstract

A brief comparison of photometric and spectrophotometric models of population synthesis is presented. Two complementary modelling in the NIR are proposed. One is a refined spectral synthesis of starbursts in the H + K band. Another model aims to predict synthetic spectra (continua and lines) and colors of starbursts and the Hubble Sequence from 220Å to 5μm.

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© 1996 Springer-Verlag Berlin Heidelberg

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Rocca-Volmerange, B. (1996). Photometric and Spectrophotometric Models in the NIR. In: Minniti, D., Rix, HW. (eds) Spiral Galaxies in the Near-IR. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-49739-4_2

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  • DOI: https://doi.org/10.1007/978-3-540-49739-4_2

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-662-22429-8

  • Online ISBN: 978-3-540-49739-4

  • eBook Packages: Springer Book Archive

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