EDP Sciences
Free Access
Volume 394, Number 1, October IV 2002
Page(s) 125 - 135
Section Formation, structure and evolution of stars
DOI https://doi.org/10.1051/0004-6361:20021096
Published online 04 October 2002

A&A 394, 125-135 (2002)
DOI: 10.1051/0004-6361:20021096

Modelling of intermediate age stellar populations III. Effects of dust-shells around AGB stars

M. Mouhcine

Observatoire Astronomique, Université L. Pasteur, CNRS UMR 7550, 11 rue de l'Université, 67000 Strasbourg, France

(Received 17 April 2002 / Accepted 29 July 2002)

In this paper we present single stellar population models of intermediate age stellar populations where dust-enshrouded Asymptotic Giant Branch (AGB) stars are introduced. The formation of carbon stars is also accounted for, and is taken to be a function of both initial stellar mass and metallicity. The effects of the dusty envelopes around AGB stars on the optical/near-infrared spectral energy distribution were introduced using semi-empirical models where the mass-loss and the photospheric chemistry determine the spectral properties of a star along the AGB sequence. The spectral dichotomy between oxygen-rich stars and carbon stars is taken into account in the modelling. We have investigated the AGB sequence morphology in the near-infrared colour-magnitude diagram as a function of time and metallicity. We show that this diagram is characterized by three morphological features, occupied by optically bright oxygen-rich stars, optically bright carbon stars, and dust-enshrouded oxygen rich and carbon stars respectively. Our models are able to reproduce the distribution of the three AGB subtype stellar populations in colour-colour diagrams. Effects of dusty envelopes on the luminosity function are also investigated. We have extended our investigations to the integrated spectro-photometric properties of stellar populations. We find that the contribution of AGB stars to the near-infrared integrated light decreases, making optical/near-infrared colours of intermediate age populations bluer than what is expected from pure photospheric emission models.

Key words: stars: AGB and post-AGB -- galaxies: star clusters -- galaxies: stellar content -- infrared: galaxies

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© ESO 2002

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