Abstract
Recent calculations of evolutionary tracks of TP-AGB stars of different mass and metallicity by Marigo et al. (2007) have been incorporated in the Bruzual & Charlot evolutionary population synthesis models. The mass of the stellar population in HUDF galaxies at z from 1 to 3 determined from fits to the spectro-photometric data of these galaxies is 50 to 80% lower than the mass determined from the BC03 models. The ages inferred for these populations are, with exceptions, 40 to 60% of the BC03 estimates. pdfS1743921307007624a. pdfissue-edsA. Vazdekis and R. F. PeletierdisplayTextSymposiumdispartContributed Papers © 2007 International Astronomical Union.
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CITATION STYLE
Bruzual, A. G. (2006). On TP-AGB stars and the mass of galaxies. In Proceedings of the International Astronomical Union (Vol. 2, pp. 125–132). Cambridge University Press. https://doi.org/10.1017/s1743921307007624
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