F.R.U.I.T.Y. - FUll-Network Repository of Updated Isotopic Tables & Yields

(1) Tabulated values refer to solar scaled metallicities ([α/Fe]=0). Thereby, if [α/Fe] is explicitly indicated, the
      metallicity of the selected models increases (e.g. the case "0.0001 [α/Fe]=0.5" has a metallicity Z=0.00024)
(2) Values in km/s
(3) Absolute ages (yr)
(4) Temporal duration of the previous interpulse phase (yr)
(5) Total stellar mass (M_¤)
(6) Mass of the H-exhausted core (M_¤)
(7) Dredged up mass during the current TDU (M_¤)
(8) Ratio between the mass of H-depleted dredged-up material (M_H)
      and the mass growth of the H-exhausted core during the previous interpulse phase
(9) maximum temperature attained at the bottom of the convective zone generated by the Thermal Pulse (TP)
(10) mean bolometric magnitude of the previous interpulse (set to zero for the first TP)
(11) logarithm of the mean surface temperature of the previous interpulse (set to zero for the first TP)
(12) logarithm of the mean surface gravity of the previous interpulse (set to zero for the first TP)
(13) Extended pockets: the inner border of the pocket is defined where v_{conv.}=10^{-11}*V_{CE} instead of 2*H_P (see Cristallo et al. 2015 ApJ, 801, 53 for details)
(14) In the Multiple case format, the query returns multiple table (depending on the number of selected models).
      Physical quantities corresponding to all TDUs are shown.
(15) In the Single case format, the query returns a single table containing all the selected models.
      Only final physical quantities can be visualized. Final composition are shown .
(16) Physical quantities at the last computed Thermal Pulse.
(17) Extrapolated physical quantities.