Comprehensive bayesian modeling of tidal circularization in open cluster binaries part I: M 35, NGC 6819, NGC 188

Tidal friction has long been recognized to circularize the orbits of binary stars over time. In this study, we use the observed distribution of orbital eccentricities in populations of binary stars to probe tidal dissipation. In contrast to previous studies, we incorporate a host of physical effects...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2022-11
Hauptverfasser:	Penev, Kaloyan M, Schussler, Joshua A
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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