J/A+AS/115/339              Stellar models VI.               (Charbonnel+, 1996)

Grid of stellar models. VI. Horizontal branch and early asymptotic giant branch for low mass stars (Z=0.020, 0.001). Charbonel C., Meynet G., Maeder A., Schaerer D. <Astron. Astrophys. Suppl. Ser. 115, 339 (1996)> =1996A&AS..115..339C 1996A&AS..115..339C
ADC_Keywords: Models, evolutionary; Abundances Keywords: stars: evolution - stars: Hertzsprung-Russel diagram - stars: AGB - stars: horizontal branch Description: New grids of models covering the evolution of low mass stars (0.8 to 1.7M☉) with metallicities Z=0.020 and 0.001 from the zero age main sequence up to the end of the early asymptotic giant branch are presented. The evolutionary tracks have been calculated with the new OPAL radiative opacities by Iglesias & Rogers (1992ApJ...397..717I 1992ApJ...397..717I) and Kurucz (1991). They complete the base of extensive grids of stellar models computed by the Geneva Group with up-to-date input physics (Schaller et al. 1992, Cat. J/A+AS/115/339; Schaerer et al. 1992, Cat. J/A+AS/98/523; Charbonnel et al. 1993, Cat. J/A+AS/101/415; Schaerer et al. 1993, Cat. J/A+AS/102/339; Meynet et al. 1994, Cat. J/A+AS/103/97). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 258 24 M=0.8, Z=0.001, no overshooting, std mass loss table2.dat 258 24 M=0.8, Z=0.020, no overshooting, std mass loss table3.dat 258 54 M=0.9, Z=0.001, no overshooting, std mass loss table4.dat 258 54 M=0.9, Z=0.020, no overshooting, std mass loss table5.dat 258 54 M=1.0, Z=0.001, no overshooting, std mass loss table6.dat 258 54 M=1.0, Z=0.020, no overshooting, std mass loss table8.dat 258 54 M=1.25, Z=0.020, no overshooting, std mass loss table9.dat 258 54 M=1.25, Z=0.001, no overshooting, std mass loss table10.dat 258 54 M=1.5, Z=0.001, with overshooting (0.20) table11.dat 258 54 M=1.5, Z=0.001, no overshooting, std mass loss table12.dat 258 54 M=1.5, Z=0.020, with overshooting (0.20) table13.dat 258 54 M=1.5, Z=0.020, no overshooting, std mass loss table14.dat 258 54 M=1.7, Z=0.001, with overshooting (0.20) table15.dat 258 54 M=1.7, Z=0.001, no overshooting, std mass loss table16.dat 258 54 M=1.7, Z=0.020, with overshooting (0.20) table17.dat 258 54 M=1.7, Z=0.020, no overshooting, std mass loss -------------------------------------------------------------------------------- Byte-by-byte Description of file: table* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- No Number of selected point 4- 17 E14.7 yr Age Age 18- 25 F8.4 solMass Mass Actual mass 27- 31 F5.3 [solLum] log(L) Luminosity 33- 37 F5.3 [K] log(Te) Effective temperature 39- 46 F8.6 --- Hs H surface abundance (mass fraction) 48- 55 F8.6 --- Hes He surface abundance (mass fraction) 57- 64 F8.6 --- C12 12C surface abundance (mass fraction) 66- 73 F8.6 --- C13 13C surface abundance (mass fraction) 75- 82 F8.6 --- N14 14N surface abundance (mass fraction) 84- 91 F8.6 --- O16 16O surface abundance (mass fraction) 93-100 F8.6 --- O17 17O surface abundance (mass fraction) 102-109 F8.6 --- O18 18O surface abundance (mass fraction) 111-118 F8.6 --- Ne20 20Ne surface abundance (mass fraction) 120-127 F8.6 --- Ne22 22Ne surface abundance (mass fraction) 129-134 F6.4 --- Mcore Core mass fraction 137-141 F5.3 [K] log(Tu) ? Uncorrected Teff (WR stars only) 144-150 F7.3 [solMass/yr] log(Mdot) Mass loss rate 152-156 F5.3 [g/cm3] log(rho) Central density 158-162 F5.3 [K] log(Tc) Central temperature 164-171 F8.6 --- Hc H central abundance (mass fraction) 173-180 F8.6 --- Hec ? He central abundance (mass fraction) 182-189 F8.6 --- C12c ? 12C central abundance (mass fraction) 191-198 F8.6 --- C13c ? 13C central abundance (mass fraction) 200-207 F8.6 --- N14c ? 14N central abundance (mass fraction) 209-216 F8.6 --- O16c ? 16O central abundance (mass fraction) 218-225 F8.6 --- O17c ? 17O central abundance (mass fraction) 227-234 F8.6 --- O18c ? 18O central abundance (mass fraction) 236-243 F8.6 --- Ne20c ? 20Ne central abundance (mass fraction) 245-252 F8.6 --- Ne22c ? 22Ne central abundance (mass fraction) -------------------------------------------------------------------------------- See also: J/A+AS/96/269 : (I) z=0.01, 0.02 (Schaller et al., 1992) J/A+AS/98/523 : (II) z=0.008 (Schaerer et al., 1992) J/A+AS/101/415 : (III) z=0.004 (Charbonnel et al., 1993) J/A+AS/102/339 : (IV) z=0.04 (Schaerer et al., 1993) J/A+AS/103/97 : (V) z=0.001, 0.004, 0.008, 0.020 and 0.040 (Meynet et al., 1994) J/A+AS/128/471 : (VII) z=0.10 (Mowlavi et al., 1998) J/A+AS/135/405 : (VIII) z=0.020, 0.001 (Charbonnel et al., 1999) Courtesy: C. Charbonnel
(End) Patricia Bauer [CDS] 12-Jan-1996
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