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J/A+AS/96/269    Stellar Models from 0.8 to 120 Msolar         (Schaller+, 1992)

New grids of stellar models from 0.8 to 120 Msolar at Z=0.020 and Z=0.001 Schaller G., Schaerer D., Meynet G., Maeder A. <Astron. Astrophys. Suppl. Ser. 96, 269 (1992)> =1992A&AS...96..269S
ADC_Keywords: Models, evolutionary ; Mass loss ; Stars, supergiant; Stars, Wolf-Rayet Keywords: stars: evolution - mass loss - supergiants - Wolf-Rayet Abstract: New grids of stellar evolutionary models covering the range of 0.8 to 120 solar masses have been computed for metallicites Z=0.020 and Z=0.001. The models use the new opacities by Rogers and Iglesias (1992ApJS...79..507R) and by Kurucz (1991) at low T. The consequent changes in the solar helium content, in the mixing length ratio and in the overshooting parameter are taken into account after careful calibrations. Important physical ingredients as the nuclear reaction rates and the neutrino loss rates have been updated. The ionization of the main heavy elements is calculated in details. Results of the models are given in a compact way at corresponding evolutionary stages in each model. In addition to the tables, we shortly present some general results on the tracks in the HR diagrams, the lifetimes in the H-, He-, C-burning phases, and on massive and WR stars. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 254 51 M=120, Z=0.020, with overshooting, standard mass loss table1a.dat 254 43 M=120, Z=0.020, with overshooting, Mdot x 2 in post-MS table2.dat 254 51 M= 85, Z=0.020, with overshooting, standard mass loss table2a.dat 254 31 M= 85, Z=0.020, with overshooting, Mdot x 2 in post-MS table3.dat 254 51 M= 60, Z=0.020, with overshooting, standard mass loss table3a.dat 254 30 M= 60, Z=0.020, with overshooting, Mdot x 2 in post-MS table4.dat 254 51 M= 40, Z=0.020, with overshooting, standard mass loss table4a.dat 254 31 M= 40, Z=0.020, with overshooting, Mdot x 2 in post-MS table5.dat 254 51 M= 25, Z=0.020, with overshooting, standard mass loss table5a.dat 254 30 M= 25, Z=0.020, with overshooting, Mdot x 2 in post-MS table6.dat 254 51 M= 20, Z=0.020, with overshooting, standard mass loss table6a.dat 254 30 M= 20, Z=0.020, with overshooting, Mdot x 2 in post-MS table7.dat 254 51 M= 15, Z=0.020, with overshooting, standard mass loss table8.dat 254 51 M= 12, Z=0.020, with overshooting, standard mass loss table9.dat 254 51 M= 9, Z=0.020, with overshooting, standard mass loss table10.dat 254 51 M= 7, Z=0.020, with overshooting, standard mass loss table11.dat 254 51 M= 5, Z=0.020, with overshooting, standard mass loss table12.dat 254 51 M= 4, Z=0.020, with overshooting, standard mass loss table13.dat 254 51 M= 3, Z=0.020, with overshooting, standard mass loss table14.dat 254 51 M=2.5, Z=0.020, with overshooting, standard mass loss table15.dat 254 51 M= 2, Z=0.020, with overshooting, standard mass loss table16.dat 254 51 M=1.7, Z=0.020, with overshooting, standard mass loss table17.dat 254 51 M=1.5, Z=0.020, with overshooting, standard mass loss table18.dat 254 51 M=1.25, Z=0.020, with overshooting, standard mass loss table19.dat 254 51 M=1.25, Z=0.020, no overshooting, standard mass loss table20.dat 254 51 M= 1, Z=0.020, no overshooting, standard mass loss table21.dat 254 17 M=0.9, Z=0.020, no overshooting, standard mass loss table22.dat 254 13 M=0.8, Z=0.020, no overshooting, standard mass loss table23.dat 254 51 M=120, Z=0.001, with overshooting, standard mass loss table24.dat 254 51 M= 85, Z=0.001, with overshooting, standard mass loss table25.dat 254 43 M= 60, Z=0.001, with overshooting, standard mass loss table26.dat 254 51 M= 40, Z=0.001, with overshooting, standard mass loss table27.dat 254 51 M= 25, Z=0.001, with overshooting, standard mass loss table28.dat 254 51 M= 20, Z=0.001, with overshooting, standard mass loss table29.dat 254 51 M= 15, Z=0.001, with overshooting, standard mass loss table30.dat 254 51 M= 12, Z=0.001, with overshooting, standard mass loss table31.dat 254 51 M= 9, Z=0.001, with overshooting, standard mass loss table32.dat 254 51 M= 7, Z=0.001, with overshooting, standard mass loss table33.dat 254 51 M= 5, Z=0.001, with overshooting, standard mass loss table34.dat 254 51 M= 4, Z=0.001, with overshooting, standard mass loss table35.dat 254 51 M= 3, Z=0.001, with overshooting, standard mass loss table36.dat 254 51 M=2.5, Z=0.001, with overshooting, standard mass loss table37.dat 254 51 M= 2, Z=0.001, with overshooting, standard mass loss table38.dat 254 51 M=1.7, Z=0.001, with overshooting, standard mass loss table39.dat 254 51 M=1.5, Z=0.001, with overshooting, standard mass loss table40.dat 254 51 M=1.25, Z=0.001,with overshooting standard mass loss table41.dat 254 51 M=1.25, Z=0.001, no overshooting, standard mass loss table42.dat 254 51 M= 1, Z=0.001, no overshooting, standard mass loss table43.dat 254 51 M=0.9, Z=0.001, no overshooting, standard mass loss table44.dat 254 14 M=0.8, Z=0.001, no overshooting, standard mass loss
Byte-by-byte Description of file: table*
Bytes Format Units Label Explanations
1- 2 I2 --- NB number of selected point 4- 17 E14.7 yr Age age 18- 25 F8.4 solMass Mass actual mass in solar masses 27- 31 F5.3 [solLum] logL log(luminosity) in solar units 33- 37 F5.3 [K] logTe log(effective temperature) 39- 46 F8.6 --- X H surface abundance (mass fraction) 48- 55 F8.6 --- Y 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) 131-136 F6.4 --- QCC core mass fraction 140-144 F5.3 [K] logTu ? log(uncorrected Teff) (WR stars only) 146-152 F7.3 [solMass/yr] logMdot log(mass loss rate) 154-158 F5.3 [g/cm3] log(rho.c) log(central density) 160-164 F5.3 [K] logTc log(central temperature) 166-173 F8.6 --- Xc H central abundance (mass fraction) 175-182 F8.6 --- Yc He central abundance (mass fraction) 184-191 F8.6 --- C12c 12C central abundance (mass fraction) 193-200 F8.6 --- C13c 13C central abundance (mass fraction) 202-209 F8.6 --- N14c 14N central abundance (mass fraction) 211-218 F8.6 --- O16c 16O central abundance (mass fraction) 220-227 F8.6 --- O17c 17O central abundance (mass fraction) 229-236 F8.6 --- O18c 18O central abundance (mass fraction) 238-245 F8.6 --- Ne20c 20Ne central abundance (mass fraction) 247-254 F8.6 --- Ne22c 22Ne central abundance (mass fraction)
Related Data: J/A+AS/98/523 (II) : z=0.008 J/A+AS/101/415 (III) : z=0.004 J/A+AS/102/339 (IV) : z=0.04 J/A+AS/103/97 (V) : z=0.001, 0.004, 0.008, 0.020, 0.040 J/A+AS/115/339 (VI) : z=0.020, 0.001 J/A+AS/128/471 (VII) : z=0.10 J/A+AS/135/405 (VIII) : z=0.020, 0.001
(End) Daniel Schaerer [Geneva Obs] 07-Sep-1993
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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