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Determination of the Inclination of Rotational Axes and Rotational Velocity from the Line Profiles of Rotating Stars

Published online by Cambridge University Press:  14 August 2015

M. Ruusalepp*
Affiliation:
Tartu Astrophysical Observatory, Estonia, USSR

Extract

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For a grid of rotating hot stars the computed line widths at the half maximum depth for the lines HeI λ 4471 and MgII λ 4481 are given. Based on the correspondent observational data the inclination of the rotational axes i and the reduced rotational velocity w have been found for 19 B and Be stars.

Type
V. Rotation and Binarity
Copyright
Copyright © Reidel 1982 

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