Abstract
We present a numerical study for the evolution of non-DA white dwarfs of 0.4, 0.55, 0.8, 1.0, and 1.2M ⊙. We pay special attention to the behaviour of the crystallization front. It is shown that crystallization begins at higher luminosities the higher the white dwarf mass is. The shape of the crystal growth function is very similar, almost independent of the value of the total stellar mass. We also study the crystallization process analytically, finding that it is nicely reproduced by a very simple model that accounts for the numerical results.
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Benvenuto, O.G.: 1988,Ph.D. thesis, Facultad de Ciencias Astronómicas y Geofísicas (UNLP).
Bergeron, P., Saffer, R.A. and Liebert, J.: 1992,Astrophys. J. 394, 228.
Chabrier, G.: 1993,Astrophys. J. 414, 695.
Chandrasekhar, S.: 1939,An introduction to the study of stellar structure, Univ. of Chicago Press.
Cox, A. and Tabor, J.: 1976,Astrophys. J. Suppl. 31, 271.
D'Antona, F. and Mazzitelli, I.: 1989,Astrophys. J. 347, 934.
D'Antona, F. and Mazzitelli, I.: 1990,Annu. Rev. Astron. Astrophys. 28, 139.
D'Antona, F. and Mazzitelli, I.: 1994,Astrophys. J. Suppl. 90, 467.
Hansen, J.P.: 1973,Phys. Rev. A 8, 3096.
Hubbard, W.B. and Lampe, M.: 1969,Astrophys. J. Suppl. 18, 297.
Iben, I.: 1975,Astrophys. J. 196, 525.
Iglesias, C.A., Rogers, F.J. and Wilson, B.G.: 1992,Astrophys. J. 397, 717.
Iglesias, C.A. and Rogers, F.J.: 1993,Astrophys. J. 412, 752.
Itoh, N. and Kohyama, Y.: 1983a,Astrophys. J. 275, 858.
Itoh, N., Mitake, S., Iyetomi, H. and Ichimaru, S.: 1983b,Astrophys. J. 273, 774.
Itoh, N., Kohyama, Y., Matsumoto, N. and Seki, M.: 1984,Astrophys. J. 285, 758.
Itoh, N., Adachi, T., Nakagawa, H., Kohyama, Y. and Munakata, H.: 1989,Astrophys. J. 339, 354.
Itoh, N., Mutoh, H. and Hikita, A.: 1992,Astrophys. J. 395, 622.
Itoh, N. and Kohyama, Y.: 1993,Astrophys. J. 404, 268.
Kippenhahn, R., Weigert, A. and Hofmeister, E.: 1967,Methods in computational Physics 7, B. Alder, S. Fernbach and M. Rottenberg (eds.), Academic Press, New York.
Koester, D. and Chanmugam, G.: 1990,Rep. Prog. Phys. 53, 837.
Kovetz, A., Lamb, D.Q. and Van Horn, H.M.: 1972,Astrophys. J. 174, 109.
Liebert, J., Dahn, C. and Monet, D.: 1988,Astrophys. J. 332, 891.
Lamb, D.Q. and Van Horn, H.M.: 1975,Astrophys. J. 200, 306.
Magni, G. and Mazzitelli, I.: 1979,Astron. and Astrophys. 72, 134.
Mestel, L.: 1952,Monthly Notices Roy. Astron. Soc. 112, 583.
Mestel, L. and Ruderman, M.A.: 1967,Monthly Notices Roy. Astron. Soc. 136, 27.
Munakata, H., Kohyama, Y. and Itoh, N.: 1987,Astrophys. J. 316, 708.
Ogata, S. and Ichimaru, S.: 1987,Phys. Rev. A 36, 5451.
Rogers, F.J. and Iglesias, C.A.: 1992,Astrophys. J. Suppl. 79, 507.
Schwarzschild, M.: 1958,Structure and Evolution of the Stars, Princeton Univ. Press.
Shapiro, S.L. and Teukolsky, S.A.: 1983,Black Holes, White Dwarfs and Neutron Stars. The Physics of Compact Objects, Wiley-Interscience, New York.
Shaviv, G. and Kovetz, A.: 1972,Astron. and Astrophys. 16, 72.
Van Horn, H.M.: 1968,Astrophys. J. 151, 227.
Wood, M.A.: 1992,Astrophys. J. 386, 539.
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Member of the Carrera del Investigador Científico, Comisión de Investigaciones Científicas de la Provincia de Buenos Aires (Argentina).
Fellow of the Consejo Nacional de Investigaciones Científicas y Técnicas (Argentina).
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Benvenuto, O.G., Althaus, L.G. White dwarf evolution and crystallization. Astrophys Space Sci 234, 11–25 (1995). https://doi.org/10.1007/BF00627278
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DOI: https://doi.org/10.1007/BF00627278