A rotational velocity υrotsini=33±3km s−1 has been measured for the Ap star HD 83368, confirming the prediction of 32 km s−1 (Kurtz) from an ‘oblique pulsator’ model

Carney, B. W.

Peterson, R. C.

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1985MNRAS.212P..33CDownloaded from https://academic.oup.com/mnras/article/212/1/33P/981254 by University of North Carolina at Chapel Hill Health Sciences Library user on 14 July 20211985MNRAS.212P..33CDownloaded from https://academic.oup.com/mnras/article/212/1/33P/981254 by University of North Carolina at Chapel Hill Health Sciences Library user on 14 July 20211985MNRAS.212P..33CDownloaded from https://academic.oup.com/mnras/article/212/1/33P/981254 by University of North Carolina at Chapel Hill Health Sciences Library user on 14 July 2021

The rotational velocity of the rapidly oscillating AP star HD 83368

https://cdr.lib.unc.edu/downloads/jq085t903

The rotational velocity of the rapidly oscillating AP star HD 83368

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