This database of tracks contains sets of tracks computed with a mass that ranges from 0.09 Msun to 14 Msun,
with six metallicity values between Z=0.004 and Z=0.017, and
with seven different values of initial rotation rate, from no rotation to the critical one.
As described in detail in Nguyen et al. 2022, each set of tracks is composed by different type of tracks. Stellar tracks with a mass above about 0.7 Msun
are the new tracks and have been computed with PARSEC v2.0. Tracks with a mass below about 0.7 Msun and horizontal branch tracks (files with the .HB
extension) are tracks from the old database, computed with PARSEC V1.2s.
The following table lists the quantities contained in the new tracks, with 0.7 Msun <= M <= 2 Msun:
Column number | Quantity | Description |
---|---|---|
1 | MODE | Model number |
2 | MASS | Current total mass [Msun] |
3 | AGE | Age [yr] |
4 | Dtime | Time-step [yr] |
5 | LOG_L | log10 total luminosity [log10 Lsun] |
6 | LOG_TE | effective temperature [log10 K] |
7 | RSTAR | Star radius [cm] |
8 | CONV | Mass of the homogeneous core (incl. overshooting) [M/Mtot] |
9 | QSCHW | Mass of the unstable core (Schwartzschild mass) [M/Mtot] |
10 | QDISC | Mass where X - Xsurface < 10-3 [M/Mtot] |
11 | QH_HE | Mass where X = 0.5*(Xmax+Xmin) [M/Mtot] |
12 | QHEL | Mass where X = 0 [M/Mtot] |
13 | Q_HE_CO | Mass where Y = 0.5*(Ymax+Ymin) [M/Mtot] |
14 | QCAROX | Mass where Y = 0 [M/Mtot] |
15 | LOG_Tc | log10 central temperature [log10 K] |
16 | LOG_RHc | log10 central density [log10 g cm-3] |
17 | LOG_Pc | log10 central pressure [log10 10-1 Pa] |
18 | PSI_C | degeneracy parameter at center |
19 | G1_AVG | Average Gamma 1 adiabatic index, see Marchant et al. 2019 |
20 | G1_AVG_CO | The same as G1_AVG but the average is calculated up to QCAROX |
21 | XCEN | central H1 mass fraction |
22 | XHE3C | central He3 mass fraction |
23 | YCEN | central He4 mass fraction |
24 | XC_CEN | central C12 mass fraction |
25 | XN_CEN | central N14 mass fraction |
26 | XO_CEN | central O16 mass fraction |
27 | XNE_CEN | central Ne20+Ne22 mass fraction |
28 | XMG_CEN | central Mg24+Mg25+Mg26 mass fraction |
29 | XSI28_CEN | central Si28 mass fraction |
30 | XS32_CEN | central S32 mass fraction |
31 | XAR36_CEN | central Ar36 mass fraction |
32 | XCA40_CEN | central Ca40 mass fraction |
33 | XTI44_CEN | central Ti44 mass fraction |
34 | DM | Mtot variation (< 0 for mass loss > for accretion) [Msun] |
35 | RATE | Mass loss or accretion rate [Msun yr-1] |
36 | M | Number of mesh points |
37 | MO1 | Last saved model, from which you can restart |
38 | OUTALF | MLT alpha coefficient |
39 | Xsup | surface H1 mass fraction |
40 | Ysup | surface He4 mass fraction |
41 | XCsup | surface C12 mass fraction |
42 | XC13sup | surface C13 mass fraction |
43 | XNsup | surface N14 mass fraction |
44 | XOsup | surface O16 mass fraction |
45 | XO18sup | surface O18 mass fraction |
46 | XNEsup | surface Ne20 + Ne22 mass fraction |
47 | XMGsup | surface Mg24 + Mg25 + Mg26 mass fraction |
48 | MU | mean molecular weight at the center |
49 | POLRAD_ENV | star polar radius [cm] |
50 | EQRAD_ENV | star equatorial radius [cm] |
51 | OMG_ENV | angular rotation rate = angular velocity / angular critical velocity |
52 | ANG_VEL_ENV | envelope angular velocity [cm s-1] |
53 | TANVEL_ENV | tangential linear velocity at the equator[cm s-1] |
54 | TOT_INERTIA | Total moment of inertia of the star [g cm2]] |
55 | TOT_ANGMOM | Total angular momentum [g cm2 s-1] |
56 | TOT_MOM_LOST | Total angular momentum lost due to stellar wind [g cm2 s-1] |
57 | VAR_MOMANG | Relative variation of Tot.Ang.Mom = (Tot_AngMom - Tot_Mom_0)/Tot_Mom_0 |
58 | R_CONV | Radius at CONV [log10 cm] |
59 | R_SCHW | Radius of the unstable core [log10 cm] |
60 | R_DISC | Radius at QDISC [log10 cm] |
61 | R_H_HE | Radius at QH_HE [log10 cm] |
62 | RHEL | Radius at QHEL [log10 cm] |
63 | R_HE_CO | Radius at Q_HE_CO [log10 cm] |
64 | R_CAROX | Radius at QCAROX [log10 cm] |
65 | TMAX | maximum temperature [log10 K] |
66 | RHTMAX | Density where T = TMAX [log10 g cm-3] |
67 | QTMAX | Mass coordinate where T = TMAX [M/Mtot] |
68 | LNUC | luminosity produced by nuclear burning [L/Ltot] |
69 | LX | luminosity by hydrogen burning [L/Ltot] |
70 | QH1 | Mass coordinate of the bottom of Hydrogen burning zone [M/Mtot] |
71 | QH2 | Mass coordinate of the top of the Hydrogen burning zone [M/Mtot] |
72 | LY | luminosity by helium burning [L/Ltot] |
73 | QHE1 | Mass coordinate of the bottom of He burning zone [M/Mtot] |
74 | QHE2 | Mass coordinate of the top of He burning zone [M/Mtot] |
75 | LC | luminosity by carbon burning [L/Ltot] |
76 | QC1 | Mass coordinate of the bottom of C burning zone [M/Mtot] |
77 | QC2 | Mass coordinate of the top of C burning zone [M/Mtot] |
78 | LNEUTR | neutrino luminosity [L/Ltot] |
79 | L_GRAV | gravitational luminosity [L/Ltot] |
80 | L_ACC | accretion luminosity [L/Ltot] |
81 | LYYY | luminosity provided by triple alpha reaction [L/Ltot] |
82 | LYC | luminosity provived by alpha capture on carbon [L/Ltot] |
83 | LYO | luminosity provided by alpha capture on oxygen [L/Ltot] |
84 | N_C | not used |
85 | AL_X_TOT | not used |
86 | EGENV_H | gravitational energy of H-rich envelope + atmosphere [log10 erg] |
87 | EGENV_HE | gravitational energy of He-rich envelope [log10 erg] |
88 | ENTAL_H | enthalpy of H-rich envelope + atmosphere [erg] |
89 | ENTAL_HE | enthalpy of He-rich envelope [erg] |
90 | E_INT_H | internal energy of H-rich envelope + atmosphere [log10 erg] |
91 | E_INT_HE | internal energy of He-rich envelope [log10 erg] |
92 | ES_TOT | total entropy [erg K-1]] |
93 | Q_CNV | depth of convective envelope [M/Mtot] |
94 | DPTH_CNV | radial depth of convective envelope [log10 cm] |
95 | TCNV_YR | turnover timescale of convective bubble [yr] |
96 | PHS | Evolutionary phase. 0 = PMS, 1 = MS, 3 = SUBG, 4 = RGB, 5 = AGB (for Mini <14) |
97 | CI1 | upper border of first conv zone [M/Mtot] |
98 | CF1 | bottom of first conv zone [M/Mtot] |
99 | CI2 | upper border of second conv zone [M/Mtot] |
100 | CF2 | bottom of second conv zone [M/Mtot] |
101 | CI3 | upper border of third conv zone [M/Mtot] |
102 | CF3 | bottom of third conv zone [M/Mtot] |
103 | CI4 | upper border of fourth conv zone [M/Mtot] |
104 | CF4 | bottom of fourth conv zone [M/Mtot] |
105 | T20L10 | atmosphere temperature of the gas at tau = 20 [log10 K] |
106 | RH20L10 | atmosphere density of the gas at tau = 20 [log10 g cm-3] |
107 | P20L10 | atmosphere pressure of the gas at tau = 20 [log10 10-1 Pa] |
108 | TE20L10 | "Effective temperature" (the one from boltzman-stefan law) at tau = 20 [log10 K] |
109 | R20L10 | atmosphere radius at tau = 20 [log10 cm] |
110 | T2_3L10 | atmosphere temperature of the gas at tau = 2/3 [log10 K] |
111 | RH2_3L10 | Atmosphere density of the gas at tau = 2/3 [log10 g cm-3] |
112 | P2_3L10 | Atmosphere pressure of the gas at tau = 2/3 [log10 10-1 Pa] |
113 | TE2_3L10 | temperature from Stefan-Boltzmann law at tau = 2/3 [log10 K] |
114 | R2_3L10 | Atmosphere radius at tau = 2/3 [log10 cm] |
115 | FIT_M | mass of the fitting point [M/Mtot] |
116 | COMP_TIME | Elapsed time (not CPU time) [s] |
The following table lists the quantities contained in the tracks, with M <= 0.7 Msun (Chen et al. 2014):
Column number | Quantity | Description |
---|---|---|
1 | MODE | Model number |
2 | MASS | Current total mass [Msun] |
3 | AGE | Age [yr] |
4 | Dtime | Time-step [yr] |
5 | LOG_L | log10 total luminosity [log10 Lsun] |
6 | LOG_TE | effective temperature [log10 K] |
7 | CONV | Mass of the homogeneous core (incl. overshooting) [M/Mtot] |
8 | QSCHW | Mass of the unstable core (Schwartzschild mass) [M/Mtot] |
9 | QDISC | Mass where X - Xsurface < 10-3 [M/Mtot] |
10 | QINTE | Mass where X = 0.5*(Xmax+Xmin) [M/Mtot] |
11 | QHEL | Mass where X = 0 [M/Mtot] |
12 | QCAROX | Mass where Y = 0 [M/Mtot] |
13 | LOG_Tc | log10 central temperature [log10 K] |
14 | LOG_RHc | log10 central density [log10 g cm-3] |
15 | LOG_Pc | log10 central pressure [log10 10-1 Pa] |
16 | QTMAX | Mass coordinate where T = TMAX [M/Mtot] |
17 | XCEN | central H1 mass fraction |
18 | XHE3C | central He3 mass fraction |
19 | YCEN | central He4 mass fraction |
20 | DM | Mtot variation (< 0 for mass loss > for accretion) [Msun] |
21 | RATE | Mass loss or accretion rate [Msun yr-1] |
22 | M | Number of mesh points |
23 | MO1 | Last saved model, from which you can restart |
24 | XC_cen | central C12 mass fraction |
25 | XO_cen | central O16 mass fraction |
26 | XN_cen | central N14 mass fraction |
27 | Rhtmax | Log10 Density where T = TMAX [Log g cm-3] |
28 | Xsup | surface H1 mass fraction |
29 | Ysup | surface He4 mass fraction |
30 | XCsup | surface C12 mass fraction |
31 | XOsup | surface O16 mass fraction |
32 | XNsup | surface N14 mass fraction |
33 | XC13sup | surface C13 mass fraction |
34 | LNUC | luminosity produced by nuclear burning [L/Ltot] |
35 | LX | luminosity by hydrogen burning [L/Ltot] |
36 | QH1 | Mass coordinate of the bottom of Hydrogen burning zone [M/Mtot] |
37 | QH2 | Mass coordinate of the top of the Hydrogen burning zone [M/Mtot] |
38 | LY | luminosity by helium burning [L/Ltot] |
39 | QHE1 | Mass coordinate of the bottom of He burning zone [M/Mtot] |
40 | QHE2 | Mass coordinate of the top of He burning zone [M/Mtot] |
41 | LC | luminosity by carbon burning [L/Ltot] |
42 | QC1 | Mass coordinate of the bottom of C burning zone [M/Mtot] |
43 | QC2 | Mass coordinate of the top of C burning zone [M/Mtot] |
44 | LNEUTR | neutrino luminosity [L/Ltot] |
45 | L_EX_LT | check [L/Ltot] |
46 | lgL_SCT | check [L/Ltot] |
47 | lgL_AC | check [L/Ltot] |
48 | lgL_AC_T | check [L/Ltot] |
49 | L_GRAV | gravitational luminosity [L/Ltot] |
50 | Rstar | Star radius [cm] |
51 | r_x | check |
52 | tau_xy | check |
53 | tau_thy | check |
54 | f_th | check |
55 | n_c | check |
56 | aL_x_tot | check |
57 | MU | mean molecular weight at the center check |
58 | MU_E | mean molecular weight for electrons at the center check |
59 | CI1 | upper border of first conv zone [M/Mtot] |
60 | CF1 | bottom of first conv zone [M/Mtot] |
61 | CI2 | upper border of second conv zone [M/Mtot] |
62 | CF2 | bottom of second conv zone [M/Mtot] |
63 | CI3 | upper border of third conv zone [M/Mtot] |
64 | CF3 | bottom of third conv zone [M/Mtot] |
65 | CI4 | upper border of fourth conv zone [M/Mtot] |
66 | CF4 | bottom of fourth conv zone [M/Mtot] |
67 | CI5 | upper border of fifth conv zone [M/Mtot] |
68 | CF5 | bottom of fifth conv zone [M/Mtot] |
69 | MFIT | mass of the fitting point [M/Mtot] check |
70 | CPU_SEC | CPU time check [s] |
The following table lists the quantities contained in the tracks, with M >= 2.0 Msun (Costa et al. 2019b):
Column number | Quantity | Description |
---|---|---|
1 | MODE | Model number |
2 | MASS | Current total mass [Msun] |
3 | AGE | Age [yr] |
4 | Dtime | Time-step [yr] |
5 | LOG_L | log10 total luminosity [log10 Lsun] |
6 | LOG_TE | effective temperature [log10 K] |
7 | Rstar | Star radius [cm] |
8 | Rpol | star polar radius [cm] |
9 | Req | star equatorial radius [cm] |
10 | OMEGA | angular rotation rate = angular velocity / angular critical velocity |
11 | Ang_vel | envelope angular velocity [cm s-1] |
12 | Vtan_eq | tangential linear velocity at the equator[cm s-1] |
13 | Mom_Iner | Total moment of inertia of the star [g cm2]] |
14 | Mom_ang | Total angular momentum [g cm2 s-1] |
15 | Mom_lost | Total angular momentum lost due to stellar wind [g cm2 s-1] |
16 | Var_MomAng | Relative variation of Tot.Ang.Mom = (Tot_AngMom - Tot_Mom_0)/Tot_Mom_0 |
17 | CONV | Mass of the homogeneous core (incl. overshooting) [M/Mtot] |
18 | QSCHW | Mass of the unstable core (Schwartzschild mass) [M/Mtot] |
19 | QDISC | Mass where X - Xsurface < 10-3 [M/Mtot] |
20 | QH_HE | Mass where X = 0.5*(Xmax+Xmin) [M/Mtot] |
21 | QHEL | Mass where X = 0 [M/Mtot] |
22 | QHE_co | Mass where X = 0.5*(Xmax+Xmin) [M/Mtot] |
23 | QCAROX | Mass where Y = 0 [M/Mtot] |
24 | LOG_Tc | log10 central temperature [log10 K] |
25 | LOG_RHc | log10 central density [log10 g cm-3] |
26 | LOG_Pc | log10 central pressure [log10 10-1 Pa] |
27 | QTMAX | Mass coordinate where T = TMAX [M/Mtot] |
28 | XCEN | central H1 mass fraction |
29 | XHE3C | central He3 mass fraction |
30 | YCEN | central He4 mass fraction |
31 | DM | Mtot variation (< 0 for mass loss > for accretion) [Msun] |
32 | RATE | Mass loss or accretion rate [Msun yr-1] |
33 | M | Number of mesh points |
34 | MO1 | Last saved model, from which you can restart |
35 | XC_cen | central C12 mass fraction |
36 | XO_cen | central O16 mass fraction |
37 | XN_cen | central N14 mass fraction |
38 | Tmax | Log10 maximum temperature [Log K ] |
39 | Xsup | surface H1 mass fraction |
40 | Ysup | surface He4 mass fraction |
41 | XCsup | surface C12 mass fraction |
42 | XOsup | surface O16 mass fraction |
43 | XNsup | surface N14 mass fraction |
44 | XC13sup | surface C13 mass fraction |
45 | LNUC | luminosity produced by nuclear burning [L/Ltot] |
46 | LX | luminosity by hydrogen burning [L/Ltot] |
47 | QH1 | Mass coordinate of the bottom of Hydrogen burning zone [M/Mtot] |
48 | QH2 | Mass coordinate of the top of the Hydrogen burning zone [M/Mtot] |
49 | LY | luminosity by helium burning [L/Ltot] |
50 | QHE1 | Mass coordinate of the bottom of He burning zone [M/Mtot] |
51 | QHE2 | Mass coordinate of the top of He burning zone [M/Mtot] |
52 | LC | luminosity by carbon burning [L/Ltot] |
53 | QC1 | Mass coordinate of the bottom of C burning zone [M/Mtot] |
54 | QC2 | Mass coordinate of the top of C burning zone [M/Mtot] |
55 | LNEUTR | neutrino luminosity [L/Ltot] |
56 | L_GRAV | gravitational luminosity [L/Ltot] |
57 | LYYY | luminosity provided by triple alpha reaction [L/Ltot] |
58 | LYC | luminosity provived by alpha capture on carbon [L/Ltot] |
59 | LYO | luminosity provided by alpha capture on oxygen [L/Ltot] |
60 | MLT | MLT alpha coefficient |
61 | n_c | check |
62 | aL_x_tot | check |
63 | XNECEN | central Ne20+Ne22 mass fraction |
64 | XNEsup | surface Ne20 + Ne22 mass fraction |
65 | XMGCEN | central Mg24+Mg25+Mg26 mass fraction |
66 | XMGsup | surface Mg24 + Mg25 + Mg26 mass fraction |
67 | MU | mean molecular weight at the center check |
68 | MU_E | mean molecular weight for electrons at the center check |
69 | R_H_HE | Radius at QH_HE [log10 cm] |
70 | RHEL | Radius at QHEL [log10 cm] |
71 | R_HE_CO | Radius at Q_HE_CO [log10 cm] |
72 | R_CAROX | Radius at QCAROX [log10 cm] |
73 | I_HE_CO | Moment of inertia within Q_HE_CO [g cm2]] |
74 | AM_HE_CO | Angular momentum within Q_HE_CO [g cm2 s-1] |
75 | I_CAROX | Moment of inertia within Q_CAROX [g cm2]] |
76 | AM_CAROX | Angular momentum within Q_CAROX [g cm2 s-1] |
77 | eg_envH | gravitational energy of H-rich envelope + atmosphere [log10 erg] |
78 | eg_encvHE | gravitational energy of He-rich envelope [log10 erg] |
79 | Q_CNV | depth of convective envelope [M/Mtot] |
80 | DPTH_CNV | radial depth of convective envelope [log10 cm] |
81 | INERT_CNV | Moment of iniertia of the convective envelope [g cm2]] |
82 | TCNV_YR | turnover timescale of convective bubble [yr] |
83 | PHS | Evolutionary phase. 0 = PMS, 1 = MS, 3 = SUBG, 4 = RGB, 5 = AGB (for Mini <14) |
84 | CI1 | upper border of first conv zone [M/Mtot] |
85 | CF1 | bottom of first conv zone [M/Mtot] |
86 | CI2 | upper border of second conv zone [M/Mtot] |
87 | CF2 | bottom of second conv zone [M/Mtot] |
88 | CI3 | upper border of third conv zone [M/Mtot] |
89 | CF3 | bottom of third conv zone [M/Mtot] |
90 | CI4 | upper border of fourth conv zone [M/Mtot] |
91 | CF4 | bottom of fourth conv zone [M/Mtot] |
92 | MFIT | mass of the fitting point [M/Mtot] check |
93 | CPU_SEC | CPU time check [s] |