6 days ago · PARSEC tracks (Bressan et al. (2012)) are computed for a scaled-solar composition and following the Y =0.2485+1.78 Z relation. The present solar metal content is Z ☉=0.0152. …

Nov 21, 2012 · parsec isochrones overlaid in the CMDs of two intermediate-age star clusters. In both cases, the distance modulus and reddening were fixed ‘by eye’ so as to reproduce the …

We present a new comprehensive collection of stellar evolutionary tracks and isochrones for rotating low- and intermediate-mass stars assembled with the updated version of parsec V2.0.

We present a new comprehensive collection of stellar evolutionary tracks and isochrones for rotating low- and intermediate-mass stars assembled with the updated version of parsec v2.0.

Sep 19, 2022 · We present a new comprehensive collection of stellar evolutionary tracks and isochrones for rotating low- and intermediate-mass stars assembled with the updated version …

Jul 18, 2022 · We present a new comprehensive collection of stellar evolutionary tracks and isochrones for rotating low- and intermediate-mass stars assembled with the updated version …

Sep 5, 2016 · For isochrones please use Leo Girardi's web interface. Tracks were run using parsec2match.py on 2016-09-05 (git hash b196c81). Download all tracks/code: All Tracks. …

We present a new comprehensive collection of stellar evolutionary tracks and isochrones for rotating low- and intermediate-mass stars assembled with the updated version of PARSEC V2.0.

We introduce a new generation of PARSEC–COLIBRI stellar isochrones that includes a detailed treatment of the thermally pulsing asymptotic giant branch (TP-AGB) phase, covering a wide …

Jan 19, 2017 · We introduce a new generation of PARSEC – COLIBRI stellar isochrones that includes a detailed treatment of the thermally pulsing asymptotic giant branch (TP-AGB) …