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Table A.1.

Description of quantities stored in the tables available at the CDS.

Stellar parameters Surface abundances Central abundances
Age t (yr) 1H 2H 1H 2H
Effective temperature log(Teff) (log(K)) 3He 4He 3He 4He
Surface luminosity log(L) (log(L)) 6Li 7Li
Surface gravothermal luminosity log(Lgrav) (log(L)) 7Be 9Be
Stellar mass M (M) 10B 11B
Photospheric radius Reff (R) 12C 13C 14C 12C 13C 14C
Photospheric density ρeff (g cm−3) 14N 15N 14N 15N
Photospheric gravity log(geff) (log(cgs)) 16O 17O 18O 16O 17O 18O
Mass-loss rate (M yr−1) 19F 19F
Central temperature log(Tc) (log(K)) 20Ne 21Ne 22Ne 20Ne 21Ne 22Ne
Central pressure Pc 23Na 23Na
Central density ρc 24Mg 25Mg 26Mg 24Mg 25Mg 26Mg
Maximum temperature Tmax (K) 26Al 27Al 26Al 27Al
Mass coordinate of Tmax (M) 28Si 28Si
Density at the location of Tmax, ρmax (g cm−3)
Central value of the total nuclear energy production rate εnuc, c (erg g−1s−1)
Central value of the gravothermal energy production rate εgrav, c (erg g−1s−1)
Central value of the plasma neutrino energy-loss rate εν, c (erg g−1s−1)
Mass at the base of CE MBCE (M)
Radius at the base of CE RBCE (R)
Temperature at the base of CE log(TBCE) (log(K))
Density at the base of CE ρBCE (g cm−3)
Mass at the top of CC MCC (M )
Radius at the top of CC RCC (R)
Temperature at the top of CC log(TCC) (log(K))
Density at the top of CC ρCC (g cm−3)
Colour
Maximum convective turnover timescale in the CE τconv, env, max (yr)
Associated Rossby number Roenv, max Bolometric magnitude
Integrated convective turnover timescale in the CE τconv, env, g (yr) Bolometric corrections
Associated Rossby number Roenv, global U − B
Convective turnover timescale at Hp/2 above the base of the CE τconv, env, Hp/2 (yr) B − V
Associated Rossby number Roenv, Hp/2 V − R
Convective turnover timescale at Hp above the base of the CE τconv, env, Hp (yr) V − I
Associated Rossby number Roenv, Hp J − K
Convective turnover timescale at mid-radius CE τconv, env, midRCE (yr) H − K
Associated Rossby number Roenv, midRCE V − K
Convective turnover timescale at mid-mass CE τconv, env, midMCE (yr) G − V
Associated Rossby number Roenv, midMCE GBP − V
Maximum convective turnover timescale in the CC τconv, core, max (yr) GRP − V
Associated Rossby number Rocore, max MU
Integrated convective turnover timescale in the CC τconv, core, g (yr) MB
Associated Rossby number Rocore, global MV
Convective turnover timescale at Hp/2 below the top of the CC τconv, core, Hp/2 (yr) MR
Associated Rossby number Rocore, Hp/2 MI
Convective turnover timescale at Hp below the top of the CC τconv, core, Hp (yr) MH
Associated Rossby number Rocore, Hp MJ
Convective turnover timescale at mid-radius CC τconv, core, midRCC (yr) MK
Associated Rossby number Rocore, midRCC MG
Convective turnover timescale at mid-mass CC τconv, core, midMCC (yr) MGBP
Associated Rossby number Rocore, midMCC MGRP
Fractional convective radius of gyration (Rucinski 1988, adimensional)
Fractional radiative radius of gyration (Rucinski 1988, adimensional)
Surface angular velocity Ωs (rad s1)
Radiative (+ convective) core mean angular velocity Ωc (rad s1)
Surface velocity vsurf (km s−1)
Surface rotation period Prot (days)
Total specific angular momentum content of the star (cgs)
Angular momentum content of the core (cgs)
Ratio Ω/Ωcrit
Break-up surface velocity (km s−1)
Angular momentum torque at the surface from magnetised stellar winds
Equipartition magnetic field according to Cranmer & Saar (2011)
The large separation from asymptotic relation Δνasymp (νHz)
The large separation from scaling relation Δνscale (νHz)
Relative error on large separation Δνerr
The frequency with the maximum amplitude νmax
Asymptotic period spacing of g-modes ΔΠ (s)
The total acoustic radius T (s)
Acoustic radius at the base of the convective envelope tBCE (s)
Acoustic radius in the helium second-ionisation region tHe (s)

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