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 are 5 to 15% of the mass determined from the BC03 models. The ages inferred for these populations are 20 to 50% of the BC03 estimates
In an attempt to constrain evolutionary models of the asymptotic giant branch (AGB) phase at the lim...
In the recent controversy about the role of thermally pulsing asymptotic giant branch (TP-AGB) stars...
6We study the debated contribution from thermally pulsing asymptotic-giant-branch (TP-AGB) stars in ...
We explore the effects of stellar population models on estimating star formation histories, ages and...
We explore the effects of using different stellar population models on estimates of star formation h...
In the recent controversy about the role of thermally pulsing asymptotic giant branch (TP-AGB) stars...
We study the debated contribution from thermally pulsing asymptotic-giant-branch (TP-AGB) stars in e...
Extended and updated grids of TP-AGB tracks have been implemented in the TRILEGAL population synthes...
In spite of its relevance, the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) phase is one of th...
Simple stellar population (SSP) synthesis models are useful tools for studying the nature of unresol...
In spite of its relevance, the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) phase is one of th...
Thermally pulsing asymptotic giant branch (TP-AGB) stars are relatively short lived (less than a few...
Thermally pulsing asymptotic giant branch (TP-AGB) stars are relatively short lived (less than a few...
In the recent controversy about the role of thermally pulsing asymptotic giant branch (TP-AGB) stars...
In an attempt to constrain evolutionary models of the asymptotic giant branch (AGB) phase at the lim...
In an attempt to constrain evolutionary models of the asymptotic giant branch (AGB) phase at the lim...
In the recent controversy about the role of thermally pulsing asymptotic giant branch (TP-AGB) stars...
6We study the debated contribution from thermally pulsing asymptotic-giant-branch (TP-AGB) stars in ...
We explore the effects of stellar population models on estimating star formation histories, ages and...
We explore the effects of using different stellar population models on estimates of star formation h...
In the recent controversy about the role of thermally pulsing asymptotic giant branch (TP-AGB) stars...
We study the debated contribution from thermally pulsing asymptotic-giant-branch (TP-AGB) stars in e...
Extended and updated grids of TP-AGB tracks have been implemented in the TRILEGAL population synthes...
In spite of its relevance, the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) phase is one of th...
Simple stellar population (SSP) synthesis models are useful tools for studying the nature of unresol...
In spite of its relevance, the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) phase is one of th...
Thermally pulsing asymptotic giant branch (TP-AGB) stars are relatively short lived (less than a few...
Thermally pulsing asymptotic giant branch (TP-AGB) stars are relatively short lived (less than a few...
In the recent controversy about the role of thermally pulsing asymptotic giant branch (TP-AGB) stars...
In an attempt to constrain evolutionary models of the asymptotic giant branch (AGB) phase at the lim...
In an attempt to constrain evolutionary models of the asymptotic giant branch (AGB) phase at the lim...
In the recent controversy about the role of thermally pulsing asymptotic giant branch (TP-AGB) stars...
6We study the debated contribution from thermally pulsing asymptotic-giant-branch (TP-AGB) stars in ...