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Asteroseismic Analysis of RY Leporis: The Post-main Sequence HADS in a Binary System

  • Authors: Wojciech Niewiadomski, Jadwiga Daszyńska-Daszkiewicz, Przemysław Walczak, Wojciech Szewczuk, Eloy Rodríguez, Piotr Kołaczek-Szymański, Aliz Derekas

Wojciech Niewiadomski et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure C1.

The histogram for parameters obtained from complex seismic modeling of the star RY Lep. Models reproduce the frequencies ν1 = 4.441626 day−1 and ν2 = 6.5991 day−1 as first and third overtone radial modes, respectively. The microturbulency velocity ξ = 4 km s−1 and the initial hydrogen abundance X0 = 0.7 are adopted.

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