Hostname: page-component-745bb68f8f-l4dxg Total loading time: 0 Render date: 2025-02-03T11:48:21.860Z Has data issue: false hasContentIssue false
  • English
  • Français

The Formation of Planetary Nebulae with Close Binary Nuclei

Published online by Cambridge University Press:  14 August 2015

J. Saltzman ,
M. Livio  and
G. Shaviv
J. Saltzman
Affiliation:
Dept. of Physics and Astronomy, Tel-Aviv University, Ramat-Aviv, ISRAEL
M. Livio
Affiliation:
Dept. of Physics and Astronomy, University of Florida, Gainesville, FL 32611
G. Shaviv
Affiliation:
Joint Institute for Laboratory Astrophysics, University of Colorado and National Bureau of Standards, Boulder, CO 80309

Extract

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.

Recent observations of nuclei of planetary nebula have shown that some of the central stars are binaries and even close binaries with periods of hours to few days.

Type
X. … and The Rest (Symbiotics, Supergiants, Planetaries, Population II Systems)
Information
Symposium - International Astronomical Union , Volume 88: Close Binary Stars: Observations and Interpretation , 1980 , pp. 571 - 573
Copyright
Copyright © Reidel 1980 

References

Kuiper, G.P.: 1941, Ap. J. 93, p. 133.Google Scholar
Lin, D.N.C.: 1977, M.N.R.A.S. 179, p. 265.CrossRefGoogle Scholar
Livio, M.: 1979, preprint.Google Scholar
Livio, N., Saltzman, J. and Shaviv, G.: 1979, M.N.R.A.S. 188, p. 1.Google Scholar
Lubow, S.H. and Shu, F.H.: 1975, Ap. J. 198, p. 383.CrossRefGoogle Scholar
Nariai, K.: 1975, Astron. Astrophys. 43, p. 309.Google Scholar
Prendergast, K.H.: 1960, Ap. J. 132, p. 162.CrossRefGoogle Scholar