Published July 22, 2021
| Version v1
Poster
Open
A-F variable stars from the northern TESS continuous viewing zone
Creators
- 1. Astronomical Institute of the Czech Academy of Sciences, Ondřejov, Czech Republic
- 2. Variable Star and Exoplanet Section, Czech Astronomical Society, Czech Republic
- 3. Institute of Physics of the Czech Academy of Sciences, Prague, Czech Republic
- 4. Central European Institute of Technology - Brno University of Technology (CEITEC BUT), Brno,Czech Republic
- 5. Department of Theoretical Physics and Astrophysics, Masaryk University, Brno, Czech Republic
Contributors
Editor:
Description
We present preliminary results of the identification of the variable stars brighter than 11 mag among A- and F-type stars in the northern TESS continuous viewing zone (CVZ). The aim of our efforts is to identify good candidates for the spectroscopic follow-up observations. We found out that about 63 % of all stars show some kind of variability. About one-third of the investigated stars shows a combination of variability types.
Files
Poster_TESS_SkarkaEtAl.pdf
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Additional details
References
- Dupret et al. (2005), A&A, 435, 927
- Murphy et al. (2014), MNRAS, 441, 2515,
- Murphy et al. (2019), MNRAS, 485, 2380
- Stassun et al. (2019), AJ, 158, 138
- Skarka et al. (2019), MNRAS, 487, 4230
- Paunzen et al. (2020), MNRAS, 499, 3976
- Watson et al. (2006), 25th Annual Symposium, The Society for Astronomical Sciences, 47