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Family links between Planetary Nebulae nuclei and cataclysmic variables, binary white dwarfs, R CrB stars, and SNe IA

Published online by Cambridge University Press:  25 May 2016

L.R. Yungelson  and
A.V. Tutukov
L.R. Yungelson
Affiliation:
Astronomical Institute of the Russian Academy of Sciences 48 Pyatnitskaya Str., 109017 Moscow, Russia
A.V. Tutukov
Affiliation:
Astronomical Institute of the Russian Academy of Sciences 48 Pyatnitskaya Str., 109017 Moscow, Russia

Abstract

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We analyse the population of PNe and links between binary PNNi and stars which are in the later evolutionary stages. In a model which assumes that all stars are born in binaries, about 16% of PN result from ejection of common envelopes in close binaries, 85% of single PNNi are formed by merger of components of binaries. In the model, 5% of PNNi may be precataclysmic binaries, 5% may be precursors of symbiotic stars, 0.4% may be pre-SN Ia, 0.1% - precursors of hydrogen-deficient giants. About 0.1% of all PNe may be hydrogen-deficient.

Type
III. Central Stars
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 85 - 90
Copyright
Copyright © Kluwer 1997 

References

Bergeron, P., Saffer, R.A., Liebert, J., 1992, ApJ, 394, 228.Google Scholar
Bragaglia, A., Renzini, A., Bergeron, P., 1995, ApJ, 443, 735.Google Scholar
Han, Z., Podsiadlowski, Ph., Eggleton, P. P., 1995, MNRAS, 800.Google Scholar
Hills, J. G., 1983, ApJ, 267, 322.Google Scholar
Iben, I. Jr., Tutukov, A. V., 1985, ApJSS, 58, 661.Google Scholar
Iben, I. Jr., Tutukov, A. V., 1993, ApJ, 418, 343.CrossRefGoogle Scholar
Iben, I. Jr., Tutukov, A. V., Yungelson, L. R., 1996, ApJ, 456, 750.Google Scholar
Iben, I. Jr., Tutukov, A. V., Yungelson, L. R., 1997, ApJ, January 20 issue.Google Scholar
King, A. et al., 1994, MNRAS, 269, 907.CrossRefGoogle Scholar
de Kool, M., 1990, ApJ, 358, 189.CrossRefGoogle Scholar
Peimbert, M. 1993, in Planetary Nebulae, eds. Weinberger, R. and Acker, A. (Dordrecht: Kluwer), 523.CrossRefGoogle Scholar
Podsiadlowski, Ph., Cannon, R. C., Rees, M. J., 1995, MNRAS, 274, 485.CrossRefGoogle Scholar
Thorne, K., Zytkow, A., 1975, ApJ, 199, L19.CrossRefGoogle Scholar
Vassiliadis, E., Wood, P., 1993, ApJ, 413, 641.Google Scholar
Yungelson, L. R., Tutukov, A. V., Livio, M., 1993, ApJ, 418, 794.Google Scholar
Yungelson, L. R. et al., 1995, ApJ, 447, 656.CrossRefGoogle Scholar
Yungelson, L. R. et al. 1996, ApJ, 466, 890.CrossRefGoogle Scholar
Zhang, C. Y., Kwok, S., 1993, ApJSS, 88, 137.Google Scholar