The FRUITY database on AGB stars: past, present and future

TL;DR

The FRUITY database provides an interactive platform for studying nucleosynthesis in AGB stars, featuring expanded models, rotation effects, and comparisons with observations to advance understanding of stellar processes.

Contribution

This paper introduces an updated, web-based database of AGB star models, including rotation effects and enhanced data, facilitating research and comparison with observational data.

Findings

Expanded AGB models across a range of masses and metallicities.

Inclusion of rotation effects in nucleosynthesis models.

Comparison of model predictions with observational data.

Abstract

We present and show the features of the FRUITY database, an interactive web-based interface devoted to the nucleosynthesis in AGB stars. We describe the current available set of AGB models (largely expanded with respect to the original one) with masses in the range 1.3<=M/M_SUN<=3.0 and metallicities -2.15<=[Fe/H]<=+0.15. We illustrate the details of our s-process surface distributions and we compare our results to observations. Moreover, we introduce a new set of models where the effects of rotation are taken into account. Finally, we shortly describe next planned upgrades.