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On the believability of polar spots
Published online by Cambridge University Press: 25 May 2016
Abstract
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Polar spots in Doppler Imaging maps of rapidly rotating late-type stars, especially the active components of RS CVn binaries, represent a major break with the solar paradigm, within which spots are only found at low latitudes. I examine critically the evidence for polar spots and point out that they are particularly sensitive to a number of systematic effects relating to determining reference “zero-points”.
- Type
- Session III: “Photospheric Phenomena: Results”
- Information
- Symposium - International Astronomical Union , Volume 176: Stellar Surface Structure , 1996 , pp. 299 - 304
- Copyright
- Copyright © Kluwer 1996
References
Rodonó, M., Cutispoto, G., Pazzani, V., Catalano, S., Byrne, P.B., Doyle, J.G., Butler, C.J., Andrews, A.D., Blanco, C., Marilli, E., Linsky, J.L., Scaltriti, F., Busso, M., Cellino, A., Hopkins, J.L., Okazaki, A., Hayashi, S.S., Zeilik, M., Helston, R., Henson, G., Smith, P., Simon, T.
1986, A&A, 165, 135
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