No CrossRef data available.
Article contents
Non-radial Pulsation Modeling of μ Centauri
Published online by Cambridge University Press: 12 April 2016
Abstract
It is shown that the line profile variability (lpv) of μ Cen can be modeled as non-radial pulsations (nrp). The use of the most recent available modeling technique for the nrp and carefully computed stellar observables (intrinsic line profile and flux) are, however, mandatory to take full advantage of present high-quality data.
- Type
- 3. Periodic Variations
- Information
- International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 228 - 231
- Copyright
- Copyright © Astronomical Society of the Pacific 2000