Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-23T03:04:36.166Z Has data issue: false hasContentIssue false
  • English
  • Français

Close-Binary Nuclei of Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

Howard E. Bond ,
Robin Ciardullo  and
Michael G. Meakes
Howard E. Bond
Affiliation:
Space Telescope Science Institute
Robin Ciardullo
Affiliation:
Pennsylvania State University
Michael G. Meakes
Affiliation:
Space Telescope Science Institute

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.

Close-binary planetary-nebula nuclei (PNNs) provide direct evidence for occurrence of a common-envelope phase in binary-star evolution. Their descendants are V471 Tauri-type detached binaries, cataclysmic binaries, and possibly Type I supernovae. Thirteen close-binary PNNs are now known from periodic photometric or radial-velocity variations, or from composite optical/UV spectra. At least 10% of PNNs are close binaries, a fraction more than sufficient to account for the formation of all of the cataclysmic variables in the solar neighborhood. The Abell 35-type binary PNNs, a class with three known members, contain rapidly rotating, chromospherically active late-type primary stars along with extremely hot companions detected with the IUE satellite.

Type
Oral and Contributed Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 517 - 521
Copyright
Copyright © Kluwer 1992 

References

Bond, H.E. 1989, in IAU Symp. No. 131, Planetary Nebulae, ed. Torres-Peimbert, S. (Dordrecht, Reidel), p. 251 CrossRefGoogle Scholar
Bond, H.E., Ciardullo, R., Fleming, T.A., and Grauer, A.D. 1989, in IAU Symp. No. 131, Planetary Nebulae, ed. Torres-Peimbert, S. (Dordrecht, Reidel), p. 310 CrossRefGoogle Scholar
Bond, H.E., Ciardullo, R., and Meakes, M.G. 1989, BAAS, 21, 789 Google Scholar
Bond, H.E., and Grauer, A.D. 1987, in IAU Colloq. No. 95, The Second Conference on Faint Blue Stars, ed. Philip, A.G.D., Hayes, D.S., and Liebert, J.W. (Schenectady, L. Davis Press), p. 221 Google Scholar
Bond, H.E., Liller, W., and Mannery, E.J. 1978, ApJ, 223, 252 Google Scholar
Bond, H.E., and Livio, M. 1990, ApJ, 355, 568 Google Scholar
Drilling, J.S. 1985, ApJ, 294, L107 Google Scholar
Drummond, J. 1980, , Google Scholar
Feibelman, W.A., and Kaler, J.B. 1983, ApJ, 269, 592 Google Scholar
Grauer, A.D., and Bond, H.E. 1983, ApJ, 271, 259 Google Scholar
Grewing, M., and Bianchi, L. 1989, in IAU Symp. No. 131, Planetary Nebulae, ed. Torres-Peimbert, S. (Dordrecht, Reidel), p. 314 CrossRefGoogle Scholar
Howarth, I.D., and Heber, U. 1990, PASP, 102, 912 CrossRefGoogle Scholar
Jacoby, G., and Gull, T. 1981, unpublished IUE observations Google Scholar
Livio, M., and Iben, I. 1992, PASP, in preparation Google Scholar
Méndez, R.H., Groth, H.G., Husfeld, D., Kudritzki, R.P., and Herrero, A. 1988a, A&A, 197, L25 Google Scholar
Méndez, R.H., Kudritzki, R.P., Herrero, A., Husfeld, D., and Groth, H.G. 1988b, A&A, 190, 113 Google Scholar
Méndez, R.H., and Niemela, V.S. 1981, ApJ, 250, 240 Google Scholar
Wallerstein, G., and Wolff, S.C. 1966, PASP, 78, 390 CrossRefGoogle Scholar
Zuckerman, B., and Aller, L.H. 1986, ApJ, 301, 772 Google Scholar