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Planetary Nebulae by Binary Nuclei

  • Mario Livio (a1)

Abstract

Planetary nebulae with close binary nuclei are reviewed. It is shown that these systems can be used as a source of information for the physics of the common envelope phase in the evolution of binary systems. Mechanisms for the production of bipolar planetary nebulae are examined and it is concluded that presently the action of binary companions to the central stars appears to provide the most promising mechanism. Other systems (e.g. novae, supernovae) in which similar processes may be operating are discussed.

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References

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Balick, B. (1987), A.J. , 94, 671.
Barden, S. C. and Wade, R. A. (1988) in A.S.P. Conference Series 3, Fiber Optics in Astronomy , ed. Barden, S. C. (San Francisco: Astron. Soc. Pacific), p. 113.
Bjorkman, J. E. and Cassinelli, J. P. (1992) in A.S.P. Conference Series 22, Nonisotropic and Variable Outflows from Stars , ed. Drissen, L. et al. (San Francisco: Astron. Soc. Pacific), p. 88.
Bond, H. E. and Livio, M. (1990) Ap. J. , 355, 568.
Bond, H. E. and Grauer, A. D. (1987) in IAU Colloq. 95, The Second Conference on Faint Blue Stars , eds. Philip, A. G. D. et al. (Schenectady: L. Davis Press), p. 221.
Bond, H. E., Ciardullo, R. and Meakes, M. G. (1992) in IAU Symp. 151, Evolutionary Processes in Interacting Binary Stars , ed. Kondo, Y. et al. (Dordrecht: Kluwer Academic Publishers), p. 577.
Drilling, J. S. (1985) Ap. J. , 294, L107.
Drummond, J. (1980) Ph.D. Thesis, New Mexico State University.
Duquennoy, A. and Mayor, M. (1991) Astr. Ap. , 248, 485.
Edwards, D. and Pringle, J. E. (1987) M.N.R.A.S. , 229, 383.
Eggleton, P. P. and Tout, C. A. (1989) Space Sci. Rev. , 50, 165.
Grauer, A. D. and Bond, H. E. 1983, Ap. J. , 271, 259.
van der Hucht, K. A. Jurriens, T. A., Olnon, F. M., The, P. S. Wesselius, P. R. and Williams, P. M. (1985) Astr. Ap. , 145, L13.
Iben, I. Jr. and Tutukov, A. V. (1984) Ap. J. Suppl. , 54, 335.
Iben, I. Jr. and Tutukov, A. V. (1989) in IAU Symp. 131, Planetary Nebulae , ed. Torres-Peimbert, S. (Dordrecht: Reidel), p. 505.
Icke, V., Balick, B. and Frank, A. (1992) Astr. Ap. , 253, 224.
Jasniewicz, G., Duquennoy, A. and Acker, A. (1987) Astr. Ap. , 180, 145.
Kahane, C., Audinos, P., Barnbaum, C. and Morris, M. (1992) preprint.
Kahn, F. D. (1982) in IAU Symp. 103, Planetary Nebulae , ed. Flower, D. R. (Dordrecht: Reidel), p. 305.
de Kool, M. (1990) Ap. J. , 358, 189.
Kwok, S. (1982) Ap. J. , 258, 280.
Livio, M., Salzman, J. and Shaviv, G. (1979) M.N.R.A.S. , 188, 1.
Livio, M. and Soker, N. (1988) Ap. J. , 329, 764.
Livio, M. and Soker, N. (1984) M.N.R.A.S. , 208, 763.
Lutz, J. H. and Lame, N. J. (1989) in IAU Symp. 131, Planetary Nebulae , ed. Torres-Peimbert, S. (Dordrecht: Reidel), p. 462.
Malasan, H. L., Yamasaki, A. and Kondo, M. (1991) A. J. , 101, 2131.
Malasan, H. L. and Yamasaki, A. (1992) preprint.
Mellema, G., Euldernik, F. and Icke, V. (1991) Astr. Ap. , 252, 718.
Mendez, R. H., Kudritzki, R. P., Herrero, A., Husfeld, D. and Groth, H. G. (1988a) Astr. Ap. , 190, 113.
Mendez, R. H., Groth, H. G., Hasfeld, D., Kudritzki, R. P. and Herrero, A. (1988b) Astr. Ap. , 197, L25.
Meyer, F. and Meyer-Hofmeister, E. (1979) Astr. Ap. , 78, 167.
Moffat, A. F. J., Lamontagne, R. and Seggewiss, W. (1982) Astr. Ap. , 114, 135.
Morris, M. (1987) PASP , 99, 1115.
Ostriker, J. P. (1975) talk presented at IAU Symp. 73, The Structure and Evolution of Close Binary Systems.
Paczynski, B. (1976) in IAU Symp. 73, The Structure and Evolution of Close Binary Systems , eds. Eggleton, P., Mitton, S. and Whelan, J. (Dordrecht: Reidel), p. 75.
Paczynski, B. and Sienkiewicz, R. (1972) Acta Astron. , 22, 73.
Paczynski, B. (1967) paper presented at IAU General Assembly, Comiss. 35.
Panagia, N., Gilmozzi, R., Macchetto, F., Adorf, H.-M., and Kirshner, R. P. 1991, Ap. J. , 380, L23.
Pascoli, G. (1990) in From Miras to Planetary Nebulae: Which Path for Stellar Evolution?” eds. Mennessier, M. D. and Omont, A. (Editions Frontieres), p. 136.
Pascoli, G., Leclerco, J. and Poulain, B. (1992) PASP , 104, 182.
Podsiadlowski, P. (1992) P.A.S.P. , in press.
Pollacco, D. L. and Bell, S. A. (1992) M.N.R.A.S. , submitted.
Prialnik, D. and Livio, M. (1985) M.N.R.A.S. , 216, 37.
Pringle, J. E. (1992) in Astrophysical Jets , eds. Burgarella, D., Livio, M. and O'Dea, C. (Cambridge: Cambridge University Press), in press.
Soker, N. (1991) Ap. J. , 367, 593.
Soker, N. (1992a) Ap. J. , 386, 190.
Soker, N. (1992b) Ap. J. , 389, 628.
Soker, N. and Livio, M. 1989, Ap. J. , 339, 268.
Soker, N. and Harpaz, A. (1992) P.A.S.P. , in press.
Taam, R. E. and Bodenheimer, P. (1989) Ap. J. , 337, 849.
Taam, R. E. and Bodenheimer, P. (1991) Ap. J. , 373, 246.
Tout, C. A. and Pringle, J. E. (1992) M.N.R.A.S. , 256, 269.
Tutukov, A. V. and Yungelson, L. R. (1979) in IAU Symp. 83, Mass Loss and the Evolution of O-Type Stars , eds. Conti, P. S. and de Loore, C. W. H. (Dordrecht: Reidel), p. 415.
Tutukov, A. V., Yungelson, L. R. and Iben, I. Jr. (1992) Ap. J. , 386, 197.
Wade, R. A. (1990) in Physics of Classical Novae , IAU Colloq. 122, eds. Cassatella, A. and Viotti, R. (Berlin: Springer-Verlag), p. 179.
Wampler, E. J., Wang, L., Baade, D., Banse, K., D'Odorico, S., Goniffes, C. and Tarenghi, M. 1990, Ap. J. , 362, L13.
Webbink, R. F. (1977) Ap. J. , 211, 486.
Webbink, R. F. (1984) Ap. J. , 277, 355.
Yungelson, L. R. (1973) Nauch Informatsii , 27, 93.
Zuckerman, B. and Gatley, I. (1988) Ap. J. , 324, 501.

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Planetary Nebulae by Binary Nuclei

  • Mario Livio (a1)

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