Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-14T18:22:12.476Z Has data issue: false hasContentIssue false
  • English
  • Français

Planetary Nebulae by Binary Nuclei

Published online by Cambridge University Press:  07 August 2017

Mario Livio
Mario Livio*
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 279 - 290
Copyright
Copyright © Kluwer 1993 

References

Balick, B. (1987), A.J. , 94, 671.CrossRefGoogle Scholar
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.Google Scholar
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.Google Scholar
Bond, H. E. and Livio, M. (1990) Ap. J. , 355, 568.CrossRefGoogle Scholar
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.Google Scholar
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.Google Scholar
Drilling, J. S. (1985) Ap. J. , 294, L107.CrossRefGoogle Scholar
Drummond, J. (1980) Ph.D. Thesis, New Mexico State University.Google Scholar
Duquennoy, A. and Mayor, M. (1991) Astr. Ap. , 248, 485.Google Scholar
Edwards, D. and Pringle, J. E. (1987) M.N.R.A.S. , 229, 383.CrossRefGoogle Scholar
Eggleton, P. P. and Tout, C. A. (1989) Space Sci. Rev. , 50, 165.CrossRefGoogle Scholar
Grauer, A. D. and Bond, H. E. 1983, Ap. J. , 271, 259.CrossRefGoogle Scholar
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.Google Scholar
Iben, I. Jr. and Tutukov, A. V. (1984) Ap. J. Suppl. , 54, 335.CrossRefGoogle Scholar
Iben, I. Jr. and Tutukov, A. V. (1989) in IAU Symp. 131, Planetary Nebulae , ed. Torres-Peimbert, S. (Dordrecht: Reidel), p. 505.CrossRefGoogle Scholar
Icke, V., Balick, B. and Frank, A. (1992) Astr. Ap. , 253, 224.Google Scholar
Jasniewicz, G., Duquennoy, A. and Acker, A. (1987) Astr. Ap. , 180, 145.Google Scholar
Kahane, C., Audinos, P., Barnbaum, C. and Morris, M. (1992) preprint.Google Scholar
Kahn, F. D. (1982) in IAU Symp. 103, Planetary Nebulae , ed. Flower, D. R. (Dordrecht: Reidel), p. 305.Google Scholar
de Kool, M. (1990) Ap. J. , 358, 189.CrossRefGoogle Scholar
Kwok, S. (1982) Ap. J. , 258, 280.CrossRefGoogle Scholar
Livio, M., Salzman, J. and Shaviv, G. (1979) M.N.R.A.S. , 188, 1.CrossRefGoogle Scholar
Livio, M. and Soker, N. (1988) Ap. J. , 329, 764.CrossRefGoogle Scholar
Livio, M. and Soker, N. (1984) M.N.R.A.S. , 208, 763.CrossRefGoogle Scholar
Lutz, J. H. and Lame, N. J. (1989) in IAU Symp. 131, Planetary Nebulae , ed. Torres-Peimbert, S. (Dordrecht: Reidel), p. 462.CrossRefGoogle Scholar
Malasan, H. L., Yamasaki, A. and Kondo, M. (1991) A. J. , 101, 2131.CrossRefGoogle Scholar
Malasan, H. L. and Yamasaki, A. (1992) preprint.Google Scholar
Mellema, G., Euldernik, F. and Icke, V. (1991) Astr. Ap. , 252, 718.Google Scholar
Mendez, R. H., Kudritzki, R. P., Herrero, A., Husfeld, D. and Groth, H. G. (1988a) Astr. Ap. , 190, 113.Google Scholar
Mendez, R. H., Groth, H. G., Hasfeld, D., Kudritzki, R. P. and Herrero, A. (1988b) Astr. Ap. , 197, L25.Google Scholar
Meyer, F. and Meyer-Hofmeister, E. (1979) Astr. Ap. , 78, 167.Google Scholar
Moffat, A. F. J., Lamontagne, R. and Seggewiss, W. (1982) Astr. Ap. , 114, 135.Google Scholar
Morris, M. (1987) PASP , 99, 1115.CrossRefGoogle Scholar
Ostriker, J. P. (1975) talk presented at IAU Symp. 73, The Structure and Evolution of Close Binary Systems. CrossRefGoogle Scholar
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.CrossRefGoogle Scholar
Paczynski, B. and Sienkiewicz, R. (1972) Acta Astron. , 22, 73.Google Scholar
Paczynski, B. (1967) paper presented at IAU General Assembly, Comiss. 35.Google Scholar
Panagia, N., Gilmozzi, R., Macchetto, F., Adorf, H.-M., and Kirshner, R. P. 1991, Ap. J. , 380, L23.CrossRefGoogle Scholar
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.Google Scholar
Pascoli, G., Leclerco, J. and Poulain, B. (1992) PASP , 104, 182.CrossRefGoogle Scholar
Podsiadlowski, P. (1992) P.A.S.P. , in press.Google Scholar
Pollacco, D. L. and Bell, S. A. (1992) M.N.R.A.S. , submitted.Google Scholar
Prialnik, D. and Livio, M. (1985) M.N.R.A.S. , 216, 37.CrossRefGoogle Scholar
Pringle, J. E. (1992) in Astrophysical Jets , eds. Burgarella, D., Livio, M. and O'Dea, C. (Cambridge: Cambridge University Press), in press.Google Scholar
Soker, N. (1991) Ap. J. , 367, 593.CrossRefGoogle Scholar
Soker, N. (1992a) Ap. J. , 386, 190.CrossRefGoogle Scholar
Soker, N. (1992b) Ap. J. , 389, 628.CrossRefGoogle Scholar
Soker, N. and Livio, M. 1989, Ap. J. , 339, 268.CrossRefGoogle Scholar
Soker, N. and Harpaz, A. (1992) P.A.S.P. , in press.Google Scholar
Taam, R. E. and Bodenheimer, P. (1989) Ap. J. , 337, 849.CrossRefGoogle Scholar
Taam, R. E. and Bodenheimer, P. (1991) Ap. J. , 373, 246.CrossRefGoogle Scholar
Tout, C. A. and Pringle, J. E. (1992) M.N.R.A.S. , 256, 269.CrossRefGoogle Scholar
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.Google Scholar
Tutukov, A. V., Yungelson, L. R. and Iben, I. Jr. (1992) Ap. J. , 386, 197.CrossRefGoogle Scholar
Wade, R. A. (1990) in Physics of Classical Novae , IAU Colloq. 122, eds. Cassatella, A. and Viotti, R. (Berlin: Springer-Verlag), p. 179.CrossRefGoogle Scholar
Wampler, E. J., Wang, L., Baade, D., Banse, K., D'Odorico, S., Goniffes, C. and Tarenghi, M. 1990, Ap. J. , 362, L13.CrossRefGoogle Scholar
Webbink, R. F. (1977) Ap. J. , 211, 486.CrossRefGoogle Scholar
Webbink, R. F. (1984) Ap. J. , 277, 355.CrossRefGoogle Scholar
Yungelson, L. R. (1973) Nauch Informatsii , 27, 93.Google Scholar
Zuckerman, B. and Gatley, I. (1988) Ap. J. , 324, 501.CrossRefGoogle Scholar