The β Cephei star HD 167743
- Author(s)
- Victoria Antoci, Gerald Handler, R R Shobbrook, Encarni Romero-Colmenero, S. Barmania, R. Spann
- Abstract
The β Cephei star HD 167743 was observed from three different observatories in the years 2006 and 2007. The data sets were collected through the filters Johnson UBV and Strömgren uvy. First analyses show six independent and five combination frequencies. We present mode identifications, which are simplified by the rather high amplitudes of the star. No evidence for rotational splitting was found yet.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Australian National University, South African Astronomical Observatory (SAAO)
- Journal
- Journal of Physics: Conference Series
- Volume
- 118
- ISSN
- 1742-6588
- DOI
- https://doi.org/10.1088/1742-6596/118/1/012045
- Publication date
- 2008
- Austrian Fields of Science 2012
- 1030 Physics, Astronomy
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/bed99323-f759-47e9-8532-2f6dcd759f3f