Hostname: page-component-7479d7b7d-c9gpj Total loading time: 0 Render date: 2024-07-09T07:25:39.146Z Has data issue: false hasContentIssue false
  • English
  • Français

Evolution of Rapidly Rotating B-Type Stars

Published online by Cambridge University Press:  12 April 2016

I. Juliana Sackmann  and
S.P.S. Anand
I. Juliana Sackmann
Affiliation:
David Dunlap Observatory, University of Toronto, Canada
S.P.S. Anand
Affiliation:
David Dunlap Observatory, University of Toronto, Canada

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 has become clear in recent years through the work of Collins (1963, 1965, 1966), Collins and Harrington (1966), Hardorp and Strittmatter (1968a, b) and Roxburgh and Strittmatter (1965) how seriously the spectrum of a star may be affected by rotation. However, before atmospheric models for rotating stars can be computed, the results of corresponding interior models have to be available. For polytropic configurations a great many rotating interior models have been constructed (Chandrasekhar, 1933; James, 1964; Stoeckly, 1965; Monaghan and Roxburgh, 1965; and Anand, 1968), but for rotating main-sequence stars few computations exist (Sweet and Roy, 1953; Roxburgh et al, 1965; Ostriker and Mark, 1968; Faulkner et al., 1968). In fact for B- and Be-type stars for which the most rapid rotation along the main sequence is observed, not a single interior model has yet been computed except in this conference reported by Kippenhahn and Thomas (1970). It is this gap that the present paper attempts to close.

Type
Part I / The Effects of Rotation on Stellar Interiors and Evolution
Information
International Astronomical Union Colloquium , Volume 4: Stellar Rotation , 1970 , pp. 63 - 72
Copyright
Copyright © Reidel 1970

References

Anand, S. P. S.: 1968, Astrophys. J. 153, 135.Google Scholar
Chandrasekhar, S.: 1933, Monthly Notices Roy. Astron. Soc. 93, 390.Google Scholar
Collins, G. W. II: 1963, Astrophys. J. 138, 1134.Google Scholar
Collins, G. W. II: 1965, Astrophys. J. 142, 265.Google Scholar
Collins, G. W. II: 1966, Astrophys. J. 146, 914.CrossRefGoogle Scholar
Collins, G. W. II and Harrington, J. P.: 1966, Astrophys. J. 146, 152.CrossRefGoogle Scholar
Faulkner, J., Roxburgh, I. W., and Strittmatter, P. A.: 1968, Astrophys. J. 151, 203.CrossRefGoogle Scholar
Hardorp, J. and Strittmatter, P. A.: 1968a, Astrophys. J. 151, 1057.Google Scholar
Hardorp, J. and Strittmatter, P. A.: 1968b, Astrophys. J. 153, 465.Google Scholar
James, R. A.: 1964, Astrophys. J. 140, 552.CrossRefGoogle Scholar
Kippenhahn, R. and Thomas, H. C.: 1970, this volume, p. 20.CrossRefGoogle Scholar
Kraft, R. P.: 1967, Astrophys. J. 150, 551.Google Scholar
Larson, R. B. and Demarque, P. R.: 1964, Astrophys. J. 140, 524.Google Scholar
Monaghan, J. J. and Roxburgh, I. W.: 1965, Monthly Notices Roy. Astron. Soc. 131, 13.Google Scholar
Ostriker, J. P. and Mark, J. W.-K.: 1968, Astrophys. J. 151, 1075 (Paper 1).Google Scholar
Roxburgh, I. W., Griffith, J. S., and Sweet, P. A.: 1965, Z. Astrophys. 61, 208.Google Scholar
Roxburgh, I. W. and Strittmatter, P. A.: 1965, Z. Astrophys 63, 15.Google Scholar
Sackmann, I. J. and Anand, S. P. S.: 1969, Astrophys. J. 155, 257.Google Scholar
Sackmann, I. J. and Anand, S. P. S.: 1970 (in press).Google Scholar
Schild, R. E.: 1966, Astrophys. J. 146, 142.Google Scholar
Schmidt-Kaler, Th.: 1964, Bonn. Veröffentl. 70, 1.Google Scholar
Stoeckly, R.: 1965, Astrophys. J. 142, 208.Google Scholar
Sweet, P. A. and Roy, A. E.: 1953, Monthly Notices Roy. Astron. Soc. 113, 701.CrossRefGoogle Scholar