Isochrones in the Gaia Era

PANEI, J. A.

Córdoba

Workshop; XII Friends of Friends Meeting; 2023

Observatorio Astronómico de Córdoba - Instituto de Astronomía Teórica

We present a set of isochrones for isolated stars with solar metallicity (Z=0.01524) for a mass range from 0.07 to 37 solar masses. The calculated bands were performed for the Gaia photometricsystem DR2 and DR3. In addition, we have calculated for other photometric systems such as Johnson’s UBVRI, 2MASS, etc. They were calculated for pre- and post-ZAMS evolutionary stages. We show evolutionary sequences from presequency to advanced stages of stellar evolution.