Flare stars in nearby Galactic open clusters based on TESS data

0548624 - ASÚ 2022 RIV SK eng J - Článek v odborném periodiku
Maryeva, Olga - Bicz, K. - Xia, C. - Baratella, M. - Čechvala, P. - Vida, K.
Flare stars in nearby Galactic open clusters based on TESS data.
Contributions of the Astronomical Observatory Skalnaté Pleso. Roč. 51, č. 1 (2021), s. 78-97. ISSN 1335-1842. E-ISSN 1336-0337
Grant CEP: GA ČR(CZ) Ga18-05665S
Institucionální podpora: RVO:67985815
Klíčová slova: galaxy * open clusters and associations * space mission
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 0.438, rok: 2021
Způsob publikování: Open access

The study is devoted to search for flare stars among confirmed members of Galactic open clusters using high-cadence photometry from TESS mission. We analyzed 957 high-cadence light curves of members from 136 open clusters. As a result, 56 flare stars were found, among them 8 hot B-A type objects. Of all flares, 63 % were detected in sample of cool stars (Teff<5000 K), and 29 % -- in stars of spectral type G, while 23 % in K-type stars and approximately 34% of all detected flares are in M-type stars. Using the FLATW'RM (FLAre deTection With Ransac Method) flare finding algorithm, we estimated parameters of flares and rotation period of detected flare stars. The flare with the largest amplitude appears on the M3 type EQ Cha star. Statistical analysis did not reveal any direct correlation between ages, rotation periods and flaring activity.
Trvalý link: http://hdl.handle.net/11104/0324662