TESS observations of 149 M dwarfs show no correlation between flare occurrence and the rotational phase of the dominant starspot, confirming an earlier K2 result with a larger sample.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Probing the Origin of Stellar Flares on M dwarfs Using TESS Data Sectors 1-3
TESS observations of 149 M dwarfs show no correlation between flare occurrence and the rotational phase of the dominant starspot, confirming an earlier K2 result with a larger sample.