Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-24T18:07:36.165Z Has data issue: false hasContentIssue false
  • English
  • Français

Peculiar Intrinsic Parameters of Massive Stars as a Result of an Early Phase of Homogeneous Evolution

Published online by Cambridge University Press:  12 April 2016

K.P. Simon
K.P. Simon*
Affiliation:
Institut für Astronomie und Astrophysik und Observatorium Wendelstein der Universität München, Scheinerstr. 1, D-8000 München

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.

Rotationallly induced mixing can explain several observational peculiarities of massive stars. Homogeneous evolution of differentially rotating stars including spindown due to stellar winds is studied by means of homology transformations of ZAMS models.

Type
V. The changing interior
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 477 - 479
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Herrero, A., Kudritzki, R.P., Vilchez, J.M., Kunze, D., Butler, K. Haser, S.: 1992, A & A, in pressGoogle Scholar
Kudritzki, R.P., Pauldrach, A., Puls, J., Abbott, D.C.: 1989, A&A 219, 205 Google Scholar
Maeder, A.: 1971, A&A 10, 354 Google Scholar
Maeder, A.: 1987, A&A 178, 159 Google Scholar
Maeder, A.: 1990, A&AS 84, 139 Google Scholar
Schõnberner, D., Herrero, A., Becker, S.,Eber, F., Butler, K., Kudritzki, R.P., Simon, K.P.: 1988, A&A 197, 209 Google Scholar
Zeipel H., von: 1924, MNRAS 84, 665 Google Scholar