Hostname: page-component-78c5997874-t5tsf Total loading time: 0 Render date: 2024-11-14T23:45:54.129Z Has data issue: false hasContentIssue false
  • English
  • Français

Evolutionary Tracks

Published online by Cambridge University Press:  07 August 2017

Detlef Schönberner
Detlef Schönberner*
Affiliation:
Institut für Theoretische Physik und Sternwarte, University of Kiel, Germany

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.

It is now accepted without any doubts that the central stars of Planetary Nebulae (CPN) are rapidly evolving objects in the transition from the asymptotic giant branch (AGB) to the white-dwarf regime. After the pioneering study of Paczyński (1971) it has been demonstrated by Schönberner (1981) that Paczyński's calculations are too crude for the understanding of post-AGB evolution because the latter depends very sensitively on the detailed internal stellar structure, i.e. on the past AGB evolution. More precisely, the evolution of an AGB remnant is a function of the thermal-pulse cycle phase ϕ during which this remnant has been created by the planetary-nebula (PN) formation process. This has been shown by Schönberner (1979, 1983) and later fully been explored by Iben (1984).

Type
V. Planetary Nebulae Connection: Evolution to White Dwarfs
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 415 - 422
Copyright
Copyright © Kluwer 1993 

References

Blöcker, T., Schönberner, D.: 1990, A&A 240, L11 Google Scholar
Blöcker, T., Schönberner, D.: 1991, A&A 244, L43 Google Scholar
Bowen, G.H.: 1988, ApJ 329, 299 Google Scholar
Härm, R., Schwarzschild, M.: 1975, ApJ 93, 200 Google Scholar
Iben, I. Jr.: 1984, ApJ 277, 333 Google Scholar
Iben, I. Jr., Kaler, J.B., Truran, J.W., Renzini, A.: 1983, ApJ 264, 605 Google Scholar
Jacoby, G.H., Kaler, J.B.: 1989, AJ 98, 1662 Google Scholar
Kaler, J.B.: 1983, ApJ 271, 188 Google Scholar
Kaler, J.B., Jacoby, G. H.: 1989, ApJ 345, 871 CrossRefGoogle Scholar
Kippenhahn, R.: 1981, A&A 102, 293 Google Scholar
Knapp, G.: 1985, ApJ 293, 273 CrossRefGoogle Scholar
Marten, H., Schönberner, D.: 1991, A&A 248, 590 Google Scholar
Ostlie, D.A., Cox, A.N.: 1986, ApJ 311, 864 Google Scholar
Paczyński, B.: 1970, Acta Astron. 20, 47 Google Scholar
Paczyński, B.: 1971, Acta Astron. 21, 417 Google Scholar
Pauldrach, A., Puls, J., Kudritzki, R.P., Méndez, R., Heap, S.R.: 1988, A&A 207, 123 Google Scholar
Perinotto, M.: 1989, IAU Symp. No. 131, Planetary Nebulae , Torres-Peimbert, S., Ed., Kluwer, p. 293 CrossRefGoogle Scholar
Reimers, D.: 1975, Problems in Stellar Atmospheres and Envelopes , Baschek, B., Kegel, W. H., Traving, G., Eds., Springer, p. 229 Google Scholar
Schönberner, D.: 1979, A&A 79, 108 Google Scholar
Schönberner, D.: 1981, A&A 103, 119 Google Scholar
Schönberner, D.: 1983, ApJ 272, 708 Google Scholar
Schönberner, D.: 1989, Proc. IAU Symp. No. 131, Planetary Nebulae , Torres-Peimbert, S., Ed., Kluwer, p. 463 Google Scholar
Schönberner, D.: 1990, Proc. Int. Coll. From Miras to Planetary Nebulae: Which Path for Stellar Evolution?, Mennessier, M. O. and Omont, A., Eds., p. 355 Google Scholar
Schönberner, D., Tylenda, R.: 1991, A&A 248, 590 Google Scholar
Schönberner, D, Blöcker, T.: 1992, Proc. Workshop Atmospheres of Early-Type Stars, Heber, U. and Jeffery, C. S., Eds., Springer, p. 305 Google Scholar
Van der Veen, W.E.C.J., Habing, H.J., Geballe, T.R.: 1989, A&A 226, 108 Google Scholar
Walton, N.A., Barlow, M.J., Clegg, R.E.S., Monk, D.J.: 1991, Proc. IAU Symp. No. 148, Magellanic Clouds, Haynes, P. R. and Milne, D. Eds., Kluwer, p. 334 Google Scholar
Weidemann, V.: 1987, A&A 188, 74 Google Scholar
Weidemann, V.: 1992, Proc. ESO-CTIO Workshop Mass Loss on the AGB and Beyond , in press Google Scholar
Wood, P.R., Faulkner, D.J.: 1986, ApJ 307, 659 Google Scholar