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Tidally distorted stars are triaxial pulsators

Title: Tidally distorted stars are triaxial pulsators
Authors: Fuller, Jim; Rappaport, Saul; Jayaraman, Rahul; Kurtz, Donald Wayne; Handler, Gerald
Publisher Information: American Astronomical Society (AAS)
Publication Year: 2025
Collection: University of Central Lancashire: CLOK - Central Lancashire Online Knowledge
Subject Terms: F510 - Astrophysics
Description: Stars in close binaries are tidally distorted, and this has a strong effect on their pulsation modes. We compute the mode frequencies and geometries of tidally distorted stars using perturbation theory, accounting for the effects of the Coriolis force and the coupling between different azimuthal orders m of a multiplet induced by the tidal distortion. For tidally coupled dipole pressure modes, the tidal coupling dominates over the Coriolis force and the resulting pulsations are ``triaxial", with each of the three modes in a multiplet ``tidally tilted" to be aligned with the one of the three principal axes of the star. The observed amplitudes and phases of the dipole modes aligned orthogonal to the spin axis are modulated throughout the orbit, producing doublets in the power spectrum that are spaced by exactly twice the orbital frequency. Quadrupole modes have similar but slightly more complex behavior. This amplitude modulation allows for mode identification which can potentially enable detailed asteroseismic analyses of tidally tilted pulsators. Pressure modes should exhibit this behavior in stellar binaries close enough to be tidally synchronized, while gravity modes should remain aligned with the star's spin axis. We discuss applications to various types of pulsating stars, and the relationship between tidal tilting of pulsations and the ``single-sided" pulsations sometimes observed in very tidally distorted stars.
Document Type: article in journal/newspaper
File Description: application/pdf
Language: English
ISSN: 0004-637X
Relation: https://clok.uclan.ac.uk/id/eprint/53793/1/53793%20Fuller%20et%20al.%20VOR.pdf; Fuller, Jim, Rappaport, Saul, Jayaraman, Rahul, Kurtz, Donald Wayne orcid iconorcid:0000-0002-1015-3268 and Handler, Gerald (2025) Tidally distorted stars are triaxial pulsators. Astrophysical Journal, 979 (1). p. 80. ISSN 0004-637X
DOI: 10.3847/1538-4357/ad9eb2
Availability: https://clok.uclan.ac.uk/id/eprint/53793/; https://clok.uclan.ac.uk/id/eprint/53793/1/53793%20Fuller%20et%20al.%20VOR.pdf; https://doi.org/10.3847/1538-4357/ad9eb2
Rights: cc_by_4
Accession Number: edsbas.FDABFC26
Database: BASE