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The ATON 3.1 stellar evolutionary code

A version for asteroseismology

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Abstract

We describe the main features of the evolutionary code ATON 3.1 and its latest version, particularly deviced to be apt for follow up asteroseismology applications. An older version of the code including rotational evolution is also shortly described.

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References

  • Allard, F., Hauschildt, P.: NextGen model sets. http://dilbert.physast.uga.edu/~yeti/mdwarfs.html (1997)

  • Angulo, C., et al.: A compilation of charged-particle induced thermonuclear reaction rates. Nucl. Phys. A 656, 3 (1999)

    Article  ADS  MathSciNet  Google Scholar 

  • Basu, S., Antia, H.M.: Seismic measurement of the depth of the solar convection zone. Mon. Not. R. Astron. Soc. 287, 189 (1997)

    ADS  Google Scholar 

  • Basu, S., Pinsonneault, M.H., Bahcall, J.N.: How much do helioseismological inferences depend on the assumed reference model? Astrophys. J. 529, 1084 (2000)

    Article  ADS  Google Scholar 

  • Böhm-Vitense, E.: Über die Wasserstoffkonvektionszone in Sternen verschiedener Effektivtemperaturen und Leuchtkräfte. Z. Astrophys. 46, 108 (1958)

    ADS  Google Scholar 

  • Canuto, V.M., Mazzitelli, I.: Stellar turbulent convection—a new model and applications. Astrophys. J. 370, 295 (1991)

    Article  ADS  Google Scholar 

  • Canuto, V.M., Goldman, I., Mazzitelli, I.: Stellar turbulent convection: a self-consistent model. Astrophys. J. 473, 550 (1996)

    Article  ADS  Google Scholar 

  • Cassisi, S., Potekhin, A.Y., Pietrinferni, A., Catelan, M., Salaris, M.: Updated electron-conduction opacities: the impact on low-mass stellar models. Astrophys. J. 661, 1094 (2007)

    Article  ADS  Google Scholar 

  • Cloutman, L.D., Eoll, J.G.: Comments on the diffusion model of turbulent mixing. Astrophys. J. 206, 548 (1976)

    Article  ADS  Google Scholar 

  • D’Antona, F., Cardini, D., Di Mauro, M.P., Maceroni, C., Mazzitelli, I., Montalbán, J.: 85 Peg A: what age for a low-metallicity solar-like star? Mon. Not. R. Astron. Soc. 363, 847 (2005)

    Article  ADS  Google Scholar 

  • Endal, A.S., Sofia, S.: The evolution of rotating stars. I—Method and exploratory calculations for a 7-solar-mass star. Astrophys. J. 210, 184 (1976)

    Article  ADS  Google Scholar 

  • Ferguson, J.W., Alexander, D.R., Allard, F., Barman, T., Bodnarik, J.G., Hauschildt, P.H., Heffner-Wong, A., Tamanai, A.: Low-temperature opacities. Astrophys. J. 623, 585 (2005)

    Article  ADS  Google Scholar 

  • Heiter, U., et al.: New grids of ATLAS9 atmospheres I: Influence of convection treatments on model structure and on observable quantities. Astron. Astrophys. 392, 619 (2002)

    Article  ADS  Google Scholar 

  • Henyey, L., Vardya, M.S., Bodenheimer, P.: Studies in stellar evolution. III. The calculation of model envelopes. Astrophys. J. 142, 841 (1965)

    Article  ADS  Google Scholar 

  • Iben, I. Jr., McDonald, J.: The effects of diffusion due to gravity and due to composition gradients on the rate of hydrogen burning in a cooling degenerate dwarf. I—The case of a thick helium buffer layer. Astrophys. J. 296, 540 (1985)

    Article  ADS  Google Scholar 

  • Iglesias, C.A., Rogers, F.J.: Updated Opal opacities. Astrophys. J. 464, 943 (1996)

    Article  ADS  Google Scholar 

  • Kippenhahn, R., Thomas, H.-C.: In: Slettebak, A. (ed.) Stellar Rotation, p. 20. Reidel, Dordrecht (1970)

    Google Scholar 

  • Landin, N.R., Ventura, P., D’Antona, F., Mendes, L.T.S., Vaz, L.P.R.: Non-gray rotating stellar models and the evolutionary history of the Orion Nebular Cluster. Astron. Astrophys. 456, 269 (2006)

    Article  ADS  Google Scholar 

  • Mazzitelli, I.: Solar models, helium content and mixing length. Astron. Astrophys. 79, 251–253 (1979)

    ADS  Google Scholar 

  • Mendes, L.T.S., D’Antona, F., Mazzitelli, I.: Theoretical models of low-mass, pre-main sequence rotating stars. I. The effects on lithium depletion. Astron. Astrophys. 341, 174 (1999)

    ADS  Google Scholar 

  • Montalbán, J., D’Antona, F., Mazzitelli, I.: Structure and evolution of low-mass Population II stars. Astron. Astrophys. 360, 935 (2000)

    ADS  Google Scholar 

  • Montalbán, J., Kupka, F., D’Antona, F., Schmidt, W.: Convection in the atmospheres and envelopes of turnoff and giant branch stars of globular clusters. Astron. Astrophys. 370, 982 (2001)

    Article  ADS  Google Scholar 

  • Montalbán, J., D’Antona, F., Kupka, F., Heiter, U.: Convection in the atmospheres and envelopes of Pre-Main Sequence stars. Astron. Astrophys. 416, 1081 (2004)

    Article  ADS  Google Scholar 

  • Paterno, L., Ventura, R., Canuto, V.M., Mazzitelli, I.: Helioseismological test of a new model for stellar convection. Astrophys. J. 402, 733 (1993)

    Article  ADS  Google Scholar 

  • Potekhin, A.Y., Baiko, D.A., Haensel, P., Yakovlev, D.G.: Transport properties of degenerate electrons in neutron star envelopes and white dwarf cores. Astron. Astrophys. 346, 345 (1999)

    ADS  Google Scholar 

  • Rogers, F.J., Nayfonov, A.: Updated and expanded OPAL equation-of-state tables: implications for helioseismology. Astrophys. J. 576, 1064 (2002)

    Article  ADS  Google Scholar 

  • Rogers, F.J., Swenson, F.J., Iglesias, C.A.: OPAL equation-of-state tables for astrophysical applications. Astrophys. J. 456, 902 (1996)

    Article  ADS  Google Scholar 

  • Saumon, D., Chabrier, G., van Horn, H.M.: An equation of state for low-mass stars and giant planets. Astrophys. J. Suppl. Ser. 99, 713 (1995)

    Article  ADS  Google Scholar 

  • Schröder, K.-P., Pols, O.R., Eggleton, P.P.: A critical test of stellar evolution and convective core ‘overshooting’ by means of zeta Aurigae systems. Mon. Not. R. Astron. Soc. 285, 696 (1997)

    ADS  Google Scholar 

  • Stolzmann, W., Blöcker, T.: Thermodynamical properties of stellar matter. I. Equation of state for stellar interiors. Astron. Astrophys. 314, 1024 (1996)

    ADS  Google Scholar 

  • Stolzmann, W., Blöcker, T.: Thermodynamical properties of stellar matter. II. Internal energy, temperature and density exponents, and specific heats for stellar interiors. Astron. Astrophys. 361, 1152 (2000)

    ADS  Google Scholar 

  • Ventura, P., Zeppieri, A., Mazzitelli, I., D’Antona, F.: Full spectrum of turbulence convective mixing: I. Theoretical main sequences and turn-off for 0.6–15M. Astron. Astrophys. 334, 953 (1998)

    ADS  Google Scholar 

  • Ventura, P., D’Antona, F., Mazzitelli, I.: Lithium and mass loss in massive AGB stars in the Large Magellanic Cloud. Astron. Astrophys. 363, 605 (2000)

    ADS  Google Scholar 

  • Ventura, P., Castellani, M., Straka, C.W.: Diffusive convective overshoot in core He-burning intermediate mass stars. I. The LMC metallicity. Astron. Astrophys. 440, 623 (2005)

    Article  ADS  Google Scholar 

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Correspondence to Francesca D’Antona.

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Ventura, P., D’Antona, F. & Mazzitelli, I. The ATON 3.1 stellar evolutionary code. Astrophys Space Sci 316, 93–98 (2008). https://doi.org/10.1007/s10509-007-9672-8

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  • DOI: https://doi.org/10.1007/s10509-007-9672-8

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