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.
Similar content being viewed by others
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)
Basu, S., Antia, H.M.: Seismic measurement of the depth of the solar convection zone. Mon. Not. R. Astron. Soc. 287, 189 (1997)
Basu, S., Pinsonneault, M.H., Bahcall, J.N.: How much do helioseismological inferences depend on the assumed reference model? Astrophys. J. 529, 1084 (2000)
Böhm-Vitense, E.: Über die Wasserstoffkonvektionszone in Sternen verschiedener Effektivtemperaturen und Leuchtkräfte. Z. Astrophys. 46, 108 (1958)
Canuto, V.M., Mazzitelli, I.: Stellar turbulent convection—a new model and applications. Astrophys. J. 370, 295 (1991)
Canuto, V.M., Goldman, I., Mazzitelli, I.: Stellar turbulent convection: a self-consistent model. Astrophys. J. 473, 550 (1996)
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)
Cloutman, L.D., Eoll, J.G.: Comments on the diffusion model of turbulent mixing. Astrophys. J. 206, 548 (1976)
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)
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)
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)
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)
Henyey, L., Vardya, M.S., Bodenheimer, P.: Studies in stellar evolution. III. The calculation of model envelopes. Astrophys. J. 142, 841 (1965)
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)
Iglesias, C.A., Rogers, F.J.: Updated Opal opacities. Astrophys. J. 464, 943 (1996)
Kippenhahn, R., Thomas, H.-C.: In: Slettebak, A. (ed.) Stellar Rotation, p. 20. Reidel, Dordrecht (1970)
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)
Mazzitelli, I.: Solar models, helium content and mixing length. Astron. Astrophys. 79, 251–253 (1979)
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)
Montalbán, J., D’Antona, F., Mazzitelli, I.: Structure and evolution of low-mass Population II stars. Astron. Astrophys. 360, 935 (2000)
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)
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)
Paterno, L., Ventura, R., Canuto, V.M., Mazzitelli, I.: Helioseismological test of a new model for stellar convection. Astrophys. J. 402, 733 (1993)
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)
Rogers, F.J., Nayfonov, A.: Updated and expanded OPAL equation-of-state tables: implications for helioseismology. Astrophys. J. 576, 1064 (2002)
Rogers, F.J., Swenson, F.J., Iglesias, C.A.: OPAL equation-of-state tables for astrophysical applications. Astrophys. J. 456, 902 (1996)
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)
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)
Stolzmann, W., Blöcker, T.: Thermodynamical properties of stellar matter. I. Equation of state for stellar interiors. Astron. Astrophys. 314, 1024 (1996)
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)
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)
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)
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)
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
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
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10509-007-9672-8