Article contents
A 10-Day Binary System Orbiting the Be Star 66 Oph
Published online by Cambridge University Press: 26 May 2016
Abstract
66 Oph is a multiple system with a close binary orbiting the B2Ve primary Be star. The binary parameters were derived by two independent methods and spectra of components BA and BB were separated by Fourier disentangling.
- Type
- Session 1 Observations of Rotating Stars
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2004
References
- 2
- Cited by