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Apparent Variation of v sin i and Rotational Modulation in Be Stars
Published online by Cambridge University Press: 26 May 2016
Abstract
v sin i was determined by applying the Fourier transform method to the line profiles of two classical Be Stars. A variation is observed in the apparent v sin i which corresponds to the main frequencies associated to nrp modes. Rotational modulation is observed in wind sensitive UV lines of the Be star ω Ori and is associated with an oblique magnetic dipole which is discovered for the first time in a classical Be star.
- Type
- Session 1 Observations of Rotating Stars
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- Copyright © Astronomical Society of the Pacific 2004