Hostname: page-component-7bb8b95d7b-qxsvm Total loading time: 0 Render date: 2024-09-12T08:27:41.971Z Has data issue: false hasContentIssue false
  • English
  • Français

Planetary Nebulae with binary nuclei

Published online by Cambridge University Press:  25 May 2016

Mario Livio
Mario Livio*
Affiliation:
Space Telescope Science Institute 3700 San Martin Drive, Baltimore, MD 21218 e-mail: mlivio@stsci.edu

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.

High resolution images of planetary nebulae have revealed a variety of non-spherical morphologies. In addition, some planetary nebulae were found to produce highly collimated jets. It is argued that binary central stars may play a crucial role in the production of all of these morphologies. In particular, a specific mechanism is identified for the generation of “point-symmetric” nebulae. It is shown that the study of binary nuclei of planetary nebulae can provide essential information for the understanding of the common envelope phase in the evolution of binary systems.

Type
III. Central Stars
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 74 - 84
Copyright
Copyright © Kluwer 1997 

References

Balick, B. 1987, A. J., 94, 671.Google Scholar
Balick, B., & Preston, H. L. 1988, A. J., 94, 958.Google Scholar
Bell, S. A., Pollacco, D. L., & Hilditch, R. W. 1994, M.N.R.A.S., 270, 449.Google Scholar
Bjorkman, J. E., & Cassinelli, J. P. 1993, Ap. J., 409, 429.Google Scholar
Bond, H. E. 1995, in Asymmetrical Planetary Nebulae, eds. Harpaz, A., & Soker, N. (Bristol: Institute of Physics Publishing), p. 61.Google Scholar
Bond, H. E., Ciardullo, R., Fullton, L. K., & Schaefer, K. G. 1996, in preparation.Google Scholar
Burrows, C. J. et al. 1996, Ap. J., in press.Google Scholar
Chevalier, R. A., & Luo, D. 1994, Ap. J., 421, 225.Google Scholar
Cliffe, J. A., Frank, A., Livio, M., & Jones, T. W. 1995, Ap. J., 447, L49.Google Scholar
Corradi, R. L. M., & Schwarz, H. E. 1993, A&A, 268, 714.Google Scholar
de Kool, M. 1990, Ap. J., 358, 189.Google Scholar
de Kool, M. 1996, in Evolutionary Processes in Binary Stars, eds. Wijers, R. A. M. J., Davies, M. B., & Tout, C. A. (Dordrecht: Kluwer), p. 365.Google Scholar
de Kool, M., & Ritter, H. 1993, A&A, 267, 397.Google Scholar
El Eid, M. F. 1994, A&A, 285, 915.Google Scholar
Frank, A., Balick, B., Icke, V., & Mellema, G. 1993, Ap. J., 404, L25.Google Scholar
Frank, A., Balick, B., & Livio, M. 1996, Ap. J., in press.Google Scholar
Harrington, J. P., & Borkowksi, K. J. 1995, presented at the 185th AAS, Tucson, AZ.Google Scholar
Harris, M. L., Lambert, D. L., & Smith, V. V. 1988, Ap. J., 325, 768.Google Scholar
Hjellming, M. S., & Taam, R. E. 1991, Ap. J., 370, 709.CrossRefGoogle Scholar
Iben, I. Jr., & Livio, M. 1993, Pub. A.S.P., 105, 1373.Google Scholar
Iben, I. Jr., & Tutukov, A. V. 1993, Ap. J., 418, 343.Google Scholar
Iben, I. Jr., & Webbink, R. F. 1989, in White Dwarfs, ed. Wegner, G. (Berlin: Springer-Verlog), p. 477.CrossRefGoogle Scholar
Icke, V., Balick, B., Frank, A. 1992, A&A, 253, 224.Google Scholar
Icke, V., Mellema, G., Balick, B., Eulderink, F., & Frank, A. 1992, Nature, 355,524.Google Scholar
Kahn, F. D. 1982, in IAU Symp. 103, Planetary Nebulae, ed. Flower, D. R. (Dordrecht: Reidel), p. 305.Google Scholar
Kwok, S. 1982, Ap. J., 258, 280.Google Scholar
Kwok, S. 1993, in Luminous High-Latitude Stars, ASP Conf. Series 45, (San Francisco: ASP), p. 348.Google Scholar
Livio, M. 1994, in Circumstellar Media in the Late Stages of Stellar Evolution, eds. Clegg, R. et al. (Cambridge: Cambridge University Press), p. 35.Google Scholar
Livio, M. 1996a, in Science with the Hubble Space Telescope-II, eds. Benvenuti, P., Macchetto, F. D., & Schreier, E. J. (Baltimore: ST ScI), p. 257.Google Scholar
Livio, M. 1996b, in Evolutionary Processes in Binary Stars, eds. Wijers, R. A. M. J., Davies, M. B., & Tout, C. A. (Dordrecht: Kluwer), p. 141.Google Scholar
Livio, M. 1996c, in IAU Colloq. 163, Accretion Phenomena & Related Objects, eds. Ferrario, L. et al., in press.Google Scholar
Livio, M., & Pringle, J. E. 1996, Ap. J., 465, L55.Google Scholar
Livio, M., & Soker, N. 1988, Ap. J., 329, 764.Google Scholar
Meixmer, M. 1993, , .Google Scholar
Mellema, G. 1995, M.N.R.A.S., 277, 173.Google Scholar
Pascoli, G., Leclercq, J., & Poulain, B. 1992, Pub. A.S.P., 104, 182.Google Scholar
Pollacco, D. L., & Bell, S. A. 1994, M.N.R.A.S., 267, 452.CrossRefGoogle Scholar
Pollacco, D. L., & Bell, S. A. 1996, private communication.Google Scholar
Prialnik, D., & Livio, M. 1985, M.N.R.A.S., 216, 37.Google Scholar
Prinlge, J. E., & Livio, M. 1996, in preparation.Google Scholar
Rasio, F. A., & Livio, M. 1996, Ap. J., 471, 366.Google Scholar
Sahai, R., & Trauger, J. T. 1996, HST press release.Google Scholar
Sarna, M. J., Dhillon, V. S., Marsh, T. R., & Marks, P. B. 1995, M.N.R.A.S., 272, L41.Google Scholar
Schwarz, H. E., Corradi, R. L. M., & Melnick, J. 1992, A&AS, 96, 23.Google Scholar
Soker, N. 1996, preprint.Google Scholar
Soker, N., & Harpaz, A. 1992, Pub. A.S.P., 104, 923.Google Scholar
Soker, N., & Livio, M. 1989, Ap. J., 339, 268.Google Scholar
Soker, N., & Livio, M. 1994, Ap. J., 421, 219.Google Scholar
Taam, R. E., & Bodenheimer, P. 1989, Ap. J., 337, 849.Google Scholar
Terman, J. L., Taam., R. E., & Hernquist, L. 1995, Ap. J., 445, 367.Google Scholar
Trammell, S. R., & Dinerstein, H. L. 1994, A. J., 108, 984.Google Scholar
Trammell, S. R., & Goodrich, R. W. 1996, Ap. J., in press.Google Scholar
Trimble, V. 1993, A&AR, 3, 1.Google Scholar
Tutukov, A. V., & Yungelson, L. R. 1979, Acta Astron., 29, 666.Google Scholar
Yungelson, L. R., Tutukov, A. V., & Livio, M. 1993, Ap. J., 418, 794.Google Scholar