Spotedness of most active flare stars detected by TESS
A new method has been proposed to determine the coverage of starspots by using periodic functions related to flare frequency. The distribution of starspots on flare stars is modeled through a von Mises circular distribution, with parameters derived from the corresponding flare frequency function. Estimates of spot coverage for the stars studied have been obtained.
Authors
- А. А. Акопян (ORCID: https://orcid.org/0000-0003-4154-0030)
Institutions
- Byurakan Astrophysical Observatory (AM)
Publication Details
- Journal
- Communications of the Byurakan Astrophysical Observatory
- Published
- 2024-12-27
- DOI
- https://doi.org/10.52526/25792776-24.71.2-268
- Citations
- 1
- Primary Topic
- Stellar, planetary, and galactic studies
- Type
- article
- Field-Weighted Citation Impact
- 0.33