Published July 22, 2021 | Version v1
Poster Open

A-F variable stars from the northern TESS continuous viewing zone

  • 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

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

Files (2.9 MB)

Name Size Download all
md5:97ec9126722f9882b050421b71b2a0d9
1.9 MB Preview Download
md5:b5c8a39f4d64781f8aeb4836c4af14d9
962.9 kB Preview Download

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