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Carbon-Oxygen White Dwarf Presupernova Models

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Supernovae: A Survey of Current Research

Part of the book series: NATO Advanced Study Institutes Series ((ASIC,volume 90))

Abstract

The long-term evolution of accreting C-O white dwarfs as a possible source of neutron stars and/or SNI events is considered. The effects of solidification of the star’s core are included, in particular carbon-oxygen separation. Different degrees of chemical differentiation and a wide range of accretion rates are studied. We determine the pre-flash configurations and we show that a variety of results are possible, ranging from total collapse to partial disruption due to off-centre ignition of carbon.

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References

  • Arnett, W.D. 1981. Private communication.

    Google Scholar 

  • Buchler, J.R., Colgate, S.A. and Mazurek, T.J. 1980. J. de Phys.Suppl. No.3, 41, C2–159.

    Google Scholar 

  • Canal, R. and Isern, J. 1979. In IAU Colloquium 53, White Dwarfs and Variable Degenerate Stars, ed. H.M. van Horn and V. Widemann (university of Rochester), p. 52.

    Google Scholar 

  • Canal, R. and Schatzman, E. 1976. Astr.Astrophys., 46, 229.

    ADS  Google Scholar 

  • Duncan, M.J., Snell, R.L., Mazurek, T.J. and Wheeler, J.C. 1976. Astrophys.Lett., 17, 19.

    ADS  Google Scholar 

  • Ergma, E.V. and Tutukov, A.V. 1976. Acta Astr., 26, 69.

    ADS  Google Scholar 

  • Mazurek, T.J., Meier, D.C. and Wheeler, J.C. 1977. Astrophys.J. 213, 518.

    Article  ADS  Google Scholar 

  • Nomoto, K. 1980. In Proc.Texas Workshop on Type I Supernovae, ed. J.C. Wheeler (Austin: University of Texas), p. 164.

    Google Scholar 

  • Nomoto, K., Sugimoto, D. and Neo, S. 1976. Astrophys.Space Sci. 39. L37.

    Article  ADS  Google Scholar 

  • Pollock, E.L. and Hansen, J.P. 1973. Phys.Rev.A., 8, 3110.

    Article  ADS  Google Scholar 

  • Stevenson, D.J. 1980. J. de Phys.Suppl., No. 3, 41, C2–53.

    Google Scholar 

  • Taam, R.E. 1980. Astrophys.J., 237, 42.

    Article  ADS  Google Scholar 

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© 1982 D. Reidel Publishing Company

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Canal, R., Isern, J., Labay, J. (1982). Carbon-Oxygen White Dwarf Presupernova Models. In: Rees, M.J., Stoneham, R.J. (eds) Supernovae: A Survey of Current Research. NATO Advanced Study Institutes Series, vol 90. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7876-8_11

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  • DOI: https://doi.org/10.1007/978-94-009-7876-8_11

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-7878-2

  • Online ISBN: 978-94-009-7876-8

  • eBook Packages: Springer Book Archive

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