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Spectral and Light Variability of Be Star 60 Cygni
Published online by Cambridge University Press: 12 April 2016
Abstract
The analysis of high S/N spectra and photometric data of 60 Cyg shows that: (1) Pronounced long-term variations in spectra are accompanied with light variations. (2) The medium-term variations of RV could indicate that 60 Cyg is a spectroscopic binary. (3) Two independent structures dominate the rapid variability of both spectrum and light of the star.
- Type
- 3. Periodic Variations
- Information
- International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 280 - 283
- Copyright
- Copyright © Astronomical Society of the Pacific 2000