First grids of low-mass stellar models and isochrones with self-consistent treatment of rotation - From 0.2 to 1.5 M⊙ at seven metallicities from PMS to TAMSL. Amard, A. Palacios, C. Charbonnel, F. Gallet, C. Georgy, N. Lagarde and L. SiessA&A, 631 (2019) A77DOI: https://doi.org/10.1051/0004-6361/201935160
