No CrossRef data available.
Article contents
Line Profile and Photometric Variations of the Be Star η Cen1
Published online by Cambridge University Press: 12 April 2016
Abstract
We review the current status of our monitoring project on Be stars. Line profile variations in Helλ667.8 nm were detected in the Be star η Cen, by means of high resolution and S/N Spectroscopic observations. They were interpreted in terms of nonradial pulsations (NRP). The fundamental parameters of η Cen obtained from BCD spectrophotometric data and interpreted using models of rapidly rotating stars, have been used to estimate the stellar rotational frequency.
- Type
- Part 2.2. B-Type Stars
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2002
Footnotes
The follow-up spectroscopic data were gathered with the 1.60m Telescope of the Observatorio do Pico dos Dias MCT/LNA (Brazil)