activity
20072021
most citedPlanet Hunters X. KIC 8462852 - Where's the Flux?

289 citations · 926 across the 20 of their papers we have counts for

collaborators

21 papers

astro-ph.SR2021★ 29 cited

Activity of TRAPPIST-1 analogue stars observed with TESS

Bálint Seli, Krisztián Vida, Attila Moór +2

As more exoplanets are being discovered around ultracool dwarfs, understanding their magnetic activity -- and the implications for habitability -- is of prime importance. To find s…

astro-ph.SR2021★ 14 cited

A confined dynamo: magnetic activity of the K-dwarf component in the pre-cataclysmic binary system V471 Tauri

Zs. Kővári, L. Kriskovics, K. Oláh +6

We scrutinize the red dwarf component in the eclipsing binary system V471 Tau in order to unravel relations between different activity layers from the stellar surface through the c…

astro-ph.SR2021

KIC 2852961 -- a superflaring red monster in the Kepler field

Zs. Kővári, K. Oláh, M. N. Günther +3

Superflares on giant stars have up to 100,000 times more energy than the high energy solar flares. However, it is disputed, whether scaling up a solar-type dynamo could explain suc…

astro-ph.SR2020★ 18 cited

Towards the true number of flaring giant stars in the Kepler field. Are there flaring specialities associated with the giant nature?

K. Oláh, Zs. Kővári, M. N. Günther +4

We aim to give a reliable estimate of the number of flaring giant stars in the Kepler field. By analyzing the flaring activity of these stars we explore their flare statistics and…

astro-ph.SR2019★ 67 cited

Flaring activity of Proxima Centauri from TESS observations: quasi-periodic oscillations during flare decay and inferences on the habitability of Proxima b

Krisztián Vida, Katalin Oláh, Zsolt Kővári +3

We analyze the light curve of the M5.5 dwarf Proxima Centauri obtained by the TESS in Sectors 11 and 12. In the day-long light curve we identified and analyzed 72 flar…

astro-ph.SR2018★ 24 cited

Cycle period, differential rotation and meridional flow for early M dwarf stars

M. Küker, G. Rüdiger, K. Oláh +1

Recent observations suggest the existence of two characteristic cycle times for early-type M stars dependent on the rotation period. They are of order one year for the fast rotator…