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The initial/final mass relation for stellar evolution with mass loss

Published online by Cambridge University Press:  12 April 2016

Volker Weidemann
Volker Weidemann*
Affiliation:
Institut f.Theoretische Physik und Sternwarte Universität Kiel, Fed.Rep. Germany

Extract

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The relation between initial and final masses is discussed under consideration of changing theoretical concepts and new empirical data on masses of white dwarfs and nuclei of planetary nebulae. It is concluded that presently adopted schemes of evolution need revision, and that no universal relation exists.

The strongest evidence for large amounts of mass loss during stellar evolution has been provided by the existence of white dwarfs – with masses typically of 0.6 m (m = M/Mʘ), much below the galactic turn-off masses – and by the phenomenon of planetary nebula production before a star descends into the white dwarf region.

Type
Session VI - Mass Loss and Stellar Evolution: Low Mass Stars
Information
International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 339 - 344
Copyright
Copyright © Reidel 1981

References

Barkat, Z.,Tuchman, Y.: 1980, Astrophys. J. 237, pp.105–110 CrossRefGoogle Scholar
Becker, S.A.,Jr.Iben, ,Icko, :1980, Astrophys.J. 237,pp.111–129 CrossRefGoogle Scholar
Feast, M.W.: 1981, Physical Processes in Red Giants, Reidel, p. 193 CrossRefGoogle Scholar
Fusi-Pecci, F.,Renzini, A.: 1976,Astron.Astrophys. 46, pp.447–454 Google Scholar
Jr,Iben, I.,Truran, J.W.: 1978,Astrophys.J. 220, pp.980–995 CrossRefGoogle Scholar
Koester, D., Schulz, V., Weidemann, V.: 1979,Astron.Astrophys.76, pp.262–275 Google Scholar
Koester, D., Weidemann, V.: 1980,Astron.Astrophys. 81, pp.145–151 Google Scholar
Kudritzki, R.P.,Reimers, D.: 1978,Astron.Astrophys.70,pp.227–239 Google Scholar
Mengel, J.G.:1976,Astron.Astrophys.48,pp.83–86 Google Scholar
Miller, G.E., Scalo, J.M.: 1979,Astrophys. J. Suppl.41, pp.513–547 CrossRefGoogle Scholar
Ostriker, J.P.,Thuan, T.X.: 1975,Astrophys.J. 202,pp.353–364 CrossRefGoogle Scholar
Reimers, D.: 1975,Mem.Soc.Roy. Sci.Liège,6th Ser.,8,pp.369–381 Google Scholar
Renzini, A: 1979,Stars and Star Systems,IAU Regional Meeting,Uppsala, Westerlund, B.E. Ed.,Reidel, D.,Dordrecht,pp.155–169 CrossRefGoogle Scholar
Renzini, A.,Voli, M.: preprint 1980 Google Scholar
Romanishin, W.,Angel, J.R.P.: 1980,Astrophys. J. 235, pp.992–998 CrossRefGoogle Scholar
Scalo, J.M.: 1976,Astrophys. J. 206,pp.215–217 CrossRefGoogle Scholar
Schönberner, D.,Weidemann, V.: Physical Processes in Red Giants,Workshop in Erice, ed. I. Iben Jr. and A. Renzini, Reidel, Dordrecht, p. 463.Google Scholar
Tuchman, Y.,Sack, N.,Barkat, Z.: 1979,Astrophys.J. 234, pp.217–227 CrossRefGoogle Scholar
Weidemann, V.: 1977,Astron.Astrophys. 59, pp.411–418 Google Scholar
Weidemannq, V.: 1978,IAU Symp.80,The HR Diagram,A.G.D.Philips,D.S.Hayes Eds. D.Reidel, Dordrecht, pp.121–124 CrossRefGoogle Scholar
Weidemann, V.,Koester, D.: 1980,Astron.Astrophys.85, pp.208–214 Google Scholar
Wood, P.R., Cahn, J.H.: 1977,Astrophys.J. 211, pp.499–508 CrossRefGoogle Scholar