MARYEVA, O., K. BICZ, Caiyun XIA, M. BARATELLA, P. ČECHVALA a K. VIDA. Flare stars in nearby Galactic open clusters based on TESS data. Contributions of the Astronomical Observatory Skalnaté Pleso. Astronomical Institute, Slovak Academy of Sciences, 2021, roč. 51, č. 1, s. 78-97. ISSN 1335-1842. Dostupné z: https://dx.doi.org/10.31577/caosp.2021.51.1.78. |
Další formáty:
BibTeX
LaTeX
RIS
@article{1764017, author = {Maryeva, O. and Bicz, K. and Xia, Caiyun and Baratella, M. and Čechvala, P. and Vida, K.}, article_number = {1}, doi = {http://dx.doi.org/10.31577/caosp.2021.51.1.78}, keywords = {Galaxy: open clusters and associations: general; stars: flare; stars: activity; space mission: TESS}, language = {eng}, issn = {1335-1842}, journal = {Contributions of the Astronomical Observatory Skalnaté Pleso}, title = {Flare stars in nearby Galactic open clusters based on TESS data}, url = {https://doi.org/10.31577/caosp.2021.51.1.78}, volume = {51}, year = {2021} }
TY - JOUR ID - 1764017 AU - Maryeva, O. - Bicz, K. - Xia, Caiyun - Baratella, M. - Čechvala, P. - Vida, K. PY - 2021 TI - Flare stars in nearby Galactic open clusters based on TESS data JF - Contributions of the Astronomical Observatory Skalnaté Pleso VL - 51 IS - 1 SP - 78-97 EP - 78-97 PB - Astronomical Institute, Slovak Academy of Sciences SN - 13351842 KW - Galaxy: open clusters and associations: general KW - stars: flare KW - stars: activity KW - space mission: TESS UR - https://doi.org/10.31577/caosp.2021.51.1.78 N2 - 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 (T-eff < 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. ER -
MARYEVA, O., K. BICZ, Caiyun XIA, M. BARATELLA, P. ČECHVALA a K. VIDA. Flare stars in nearby Galactic open clusters based on TESS data. \textit{Contributions of the Astronomical Observatory Skalnaté Pleso}. Astronomical Institute, Slovak Academy of Sciences, 2021, roč.~51, č.~1, s.~78-97. ISSN~1335-1842. Dostupné z: https://dx.doi.org/10.31577/caosp.2021.51.1.78.
|