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Spectral synthesis in the near UV (3000–4500 Å)

Published online by Cambridge University Press:  01 December 2006

Rodolfo Smiljanic  and
Beatriz Barbuy
Rodolfo Smiljanic
Affiliation:
Universidade de São Paulo, IAG, Rua do Matão 1226, 05508-090, São Paulo SP, Brazil email: rodolfo@astro.iag.usp.br, barbuy@astro.iag.usp.br European Southern Observatory – Garching bei München
Beatriz Barbuy
Affiliation:
Universidade de São Paulo, IAG, Rua do Matão 1226, 05508-090, São Paulo SP, Brazil email: rodolfo@astro.iag.usp.br, barbuy@astro.iag.usp.br
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Abstract

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In this work we review the details, with emphasis on the near UV (3000-4500 Å), of the molecular database and the continuous opacity sources as implemented in the spectrum synthesis code used to calculate the spectral library presented in Coelho et al. (2005). We discuss our recent and future efforts towards the improvement of the calculation in this spectral range.

Keywords

atomic datamolecular dataultraviolet: stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 103 - 104
Copyright
Copyright © International Astronomical Union 2007

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