No CrossRef data available.
Article contents
Apparent Variation of v sin i and Rotational Modulation in Be Stars
Published online by Cambridge University Press: 26 May 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2004
References
Gray, D.F.
1976, in The observation and analysis of stellar photospheres, John Wiley & Sons, Inc.
Google Scholar
Neiner, C., Hubert, A.M., Frémat, Y., Floquet, M., Jankov, S. et al. 2003, A&A
409, 275
Google Scholar
You have
Access