A new parameter, DDM, derived from recurrence patterns in Kepler light curves, offers an alternative classification of close binary stars based on nonlinear dynamics.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data
A new parameter, DDM, derived from recurrence patterns in Kepler light curves, offers an alternative classification of close binary stars based on nonlinear dynamics.