"The progenitor of binary millisecond radio pulsar PSR J1713+0747
(Research Note)"
Chen, W-C. and Panei, J. A., arXiv:1101.5343
Evolutionary tracks after mass transfered has finished.
m0.30578.trk
m0.30630.trk
m0.30667.trk
m0.30675.trk
m0.30679.trk
m0.30694.trk
m0.30704.trk
Columns for files with extension: trk
1: Log(L) is Log10(L/L_sun)
2: Log(Teff) is Log10(Teff[K])
3: T_c is Log10(central temperature in units of 10**6 K)
4: Rho_c is log10(central density)
5: Hc is central abundance of H1
6: Hec is central abundance of He4
7: %Con_s is superficial convection (porcentual)
8: %Con_c is central convection (porcentual)
9: Log(age/Myr) is Log10(age in Myr units).
when mass transfered has finished we set age=0.0 Myr
10: Mass is M_WD/M_sun
11: M^dot is dM/dt (mass loss)
12: #model is the model number
13: Log(Lpp) is Log10(integrated luminosity by p-p cycle in L_sun units)
14: Log(Lcno) is Log10(integrated luminosity by CNO cycle in L_sun units)
15: Log(LHe) is Log10(integrated luminosity by He-burning in L_sun units)
16 Log(LCC) is Log10(integrated luminosity by C-burning in L_sun units)
17: int(dS/dt) is d(entropy S)/dt (integrated)
18: Log(Lnu) is Log10(integrated luminosity by neutrino in L_sun units)
19: Log MHtot is log10(total mass of H in star in M_sun units)
20: Log HeBuf is Log10(helium buffer)
21: Mass_HFC is integrated mass for H free core in M_sun units (it is He-core)
22: Mass_HeFC is integrated mass for He free core in M_sun units