Spectroscopic detection of Altair's non-radial pulsations
M. Rieutord, P. Petit, D. Reese, T. B\"ohm, A. Lopez Ariste, G., Mirouh, A. Domiciano de Souza

TL;DR
This study uses high-resolution spectroscopy to detect and analyze gravito-inertial waves in the rapidly rotating star Altair, providing new observational constraints on its oscillation modes and stellar properties.
Contribution
First detection of gravito-inertial waves in Altair through spectroscopic observations, advancing understanding of oscillations in fast rotating stars.
Findings
Detected line profile variations indicating surface waves
Identified gravito-inertial waves with azimuthal wavenumbers m=10-15
First modeling of observed waves using recent stellar models
Abstract
Context: Rapid rotation is a common feature of early-type stars but which remains a challenge for the models. The understanding of its effect on stellar evolution is however imperative to interpret the observed properties of numerous stars. Aims: We wish to bring more observational constraints on the properties of fast rotating stars, especially on their oscillation modes. Methods: We focus on the nearby star Altair which is known as a very rapidly rotating star with an equatorial velocity estimated recently at 313 km/s. We observed this star with the high-resolution spectropolarimeter Neo-Narval during six nights, with one night of interruption, in September 2020. Results: We detect significant line profile variations on the mean line profile of the spectra. Their time-frequency analysis shows that these variations are induced by gravito-inertial waves propagating at Altair's surface…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Geophysics and Sensor Technology
