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The Problem of Uniqueness in Doppler Imaging

Published online by Cambridge University Press:  12 April 2016

M. Al-Malki  and
Z. Eker
M. Al-Malki
Affiliation:
King Saud University, Science College, Department of Astronomy, P.O. Box 2455, Riyadh 11451, Saudi Arabia
Z. Eker
Affiliation:
King Saud University, Science College, Department of Astronomy, P.O. Box 2455, Riyadh 11451, Saudi Arabia

Abstract

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The uniqueness problem in Doppler imaging is discussed. Most of the problem appears to be confusion between different meanings of the word “uniqueness”. According to specific definitions presented in this study, there should not be any uniqueness problem.

Type
Part 6. Stellar Rotation, Doppler Imaging
Information
International Astronomical Union Colloquium , Volume 170: Precise Stellar Radial Velocities , 1999 , pp. 255 - 258
Copyright
Copyright © Astronomical Society of the Pacific 1999

References

Budding, E., & Zeilik, M. 1987, ApJ, 319, 827 CrossRefGoogle Scholar
Lyon, R.G., Hollis, J.M., & Dorband, J.E. 1997, ApJ, 478, 658 Google Scholar
Skilling, J., & Bryan, R.J. 1984, MNRAS, 211, 111 Google Scholar
Vogt, S.S., Penrod, G.D., & Hatzes, A.P. 1987, ApJ, 321, 496 Google Scholar