VizieR Online Data Catalog: Convective-core overshooting of massive stars (Temaj+, 2024)

Properties of all our models used throughout the paper. Explosion properties of models that were not computed to core-collapse are empty. We give the initial masses Mini, convective core overshooting values αov, helium-core masses MHe, CO-core masses MCO, iron-core masses MFe, carbon abundance at the end of core-helium burning XC, final mass of the models Mfinal, compactness value {chi}2.5, central specific entropy at the onset of iron-core collapse sc, the gravitational binding energy of the material above the iron core -Ebind, the predicted final fate, the gravitational remnant masses Mrm, explosion energy Eexpl, kick velocity vkick, nickel mass MNi, ejecta mass M_ej, plateau luminosity Lp/Lp,0, duration of the plateau tp/tp,0, luminosity at the end of core-helium burning logLc and the effective temperature at the end of core-helium burning logTeff.

(1 data file).