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Table 3
Comparison among recent databases.
Models | Present models (Pisa) | BaSTI (Teramo) | STEV(Padova) | Dartmouth |
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Mass range [M⊙] | 0.30 ÷ 1.10 | 0.50 ÷ 10.0 | 0.15 ÷ 20.0 | 0.10 ÷ 4.00 |
Metallicity (Z) | 1 × 10-4 ÷ 1 × 10-2 | 1 × 10-4 ÷ 4 × 10-2 | 1 × 10-4 ÷ 7 × 10-2 | [Fe/H] = − 2.5 ÷ 0.5 |
Helium abundance (Y) | 0.25; 0.27; 0.33; 0.38; 0.42; | 0.245 ≤ Y ≤ 0.303 | 0.23; 0.26; 0.30; 0.34; | 0.33; 0.40; |
Y = 0.2485 + 2Z | Y = 0.245 + 1.4Z | 0.40; 0.46 * | Y = 0.245 + 1.6Z | |
Solar mixture | AGSS09a | GN93b | GN93b | GS98c |
[α/Fe] | 0.0; +0.3 | +0.4 | 0.0 | −0.2 ÷ + 0.8 ([Fe/H] ≤ 0) |
−0.2 ÷ + 0.2 ([Fe/H] > 0)** | ||||
Evolutionary phases | PMS; H+He | PMS; H+He | H+He | PMS; H+He |
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αml | 1.70; 1.80; 1.90 | 1.913 | 1.68 | 1.938 |
Diffusion | Thoul et al. (1994) | NO | NO | Thoul et al. (1994) |
Mmin for overshoot | NO overshooting | 1.1 M⊙ | 1.1 M⊙ | 1.1 M⊙ |
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EOS | OPAL2006+Straniero (1988) | FreeEOSA | Bertelli et al. (2008)+ | Chaboyer & Kim (1995)+ |
Mihalas et al. (1990) | FreeEOSA | |||
Radiative opacity | OPAL2006+F05d | OPAL96+F05d | OPAL96+AF94e | OPAL96+F05d |
Conductive opacity | Cassisi et al. (2007) | Potekhin (1999) | Itoh et al. (1983) | Hubbard & Lampe (1969) |
Potekhin et al. (1999) | ||||
Reactions rates | NACRE | NACRE | Caughlan & Fowler (1988) | Adelberger et al. (1998) |
Imbriani et al. (2005)f | Imbriani et al. (2004)f | |||
Hammer et al. (2005)g | Kunz et al. (2002)g | Kunz et al. (2002)g | ||
Cyburt & Davids (2008)h | Landre et al. (1990)i | |||
Neutrinos | Haft et al. (1994) | Haft et al. (1994) | Haft et al. (1994) | Haft et al. (1994) |
Itoh et al. (1996) | ||||
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Boundary conditions | Brott & Hauschildt (2005) | Krishna Swamy (1966) | Castelli & Kurucz (2003) | Hauschildt et al. (1999) |
Castelli & Kurucz (2003) | Castelli & Kurucz (2003) |
Notes.
(a)
AGSS09 = Asplund et al. (2009).
(b)
GN93 = Grevesse & Noels (1993).
(c)
GS98 = Grevesse & Sauval (1998).
(d)
F05 = Ferguson et al. (2005).
(e)
AF94 = Alexander & Ferguson (1994).
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