Hostname: page-component-7479d7b7d-767nl Total loading time: 0 Render date: 2024-07-12T07:29:04.989Z Has data issue: false hasContentIssue false
  • English
  • Français

The Surface Distribution of Chemical Anomalies of Ap Components in Detached Close Binaries

Published online by Cambridge University Press:  14 August 2015

M. Kitamura
M. Kitamura*
Affiliation:
Tokyo Astronomical Observatory University of Tokyo, Mitaka Tokyo 181, Japan

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.

By estimating the orbital inclinations of non-eclipsing detached close binaries with Ap spectra, a marked statistical preference is obtained on the frequency distribution of the inclination which suggests that the abundance anomalies of Ap components tend to concentrate towards the stellar polar region.

Type
II. Detached Systems
Information
Symposium - International Astronomical Union , Volume 88: Close Binary Stars: Observations and Interpretation , 1980 , pp. 95 - 99
Copyright
Copyright © Reidel 1980 

References

Abt, H.A. and Bidelman, W.P.: 1969, Astrophys. J., 158, 1091.CrossRefGoogle Scholar
Batten, A.H., Fletcher, J.M. and Mann, P.J.: 1978, Publ. Dominion Astrophys. Obs., 13, No. 8, 119.Google Scholar
Dworetsky, M.: 1975, In Weiss, W. W., Jenkner, H. and Wood, H.J. (ed.), Physics of Ap Stars (IAU Coll. No. 32), Wien Univ. Obs., p. 228.Google Scholar
Kitamura, M. and Kondo, M.: 1978, Astrophys. Sp. Sci., 56, 341.CrossRefGoogle Scholar
Kitamura, M.: 1980, Astrophys. Space Sci., 68, 283.CrossRefGoogle Scholar