Pulsational stability of the SX Phe star AE UMa
Abstract
From newly determined times of maxima of the SX Phe star AE UMa and a compilation of previous times of maxima, we were able to determine the nature of this star. With uv photometry we determined its physical parameters.
- Publication:
-
Information Bulletin on Variable Stars
- Pub Date:
- November 2016
- DOI:
- 10.22444/IBVS.6186
- Bibcode:
- 2016IBVS.6186....1P