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The Rotation of the Ap Stars from the Point of View of the Rigid Rotator Model
[chapter]
1970
Stellar Rotation
Deutsch's period vs. line-width relation for the periodic Ap stars is re-examined from the point of view of the rigid rotator with the aid of recently determined values of v sin i for these objects. The agreement between computed rotational velocities and observed values of v sin / is satisfactory if the radii of the Ap stars are twice those of zero-age main sequence stars of the same color. The computed rotational velocities also agree with the mean rotational velocities of all Ap stars if
doi:10.1007/978-94-010-3299-5_28
fatcat:5q34x4oc2ncixf2gfnqhkspcfm