An improved asteroseismic age of the rapid rotator Altair from TESS data
Michel Rieutord, Daniel R. Reese, Joey S. G. Mombarg, St\'ephane, Charpinet

TL;DR
This study refines the age of the fast-rotating star Altair using new asteroseismic data from TESS, combining 1D and 2D stellar models to achieve a more precise age estimate of 88±10 million years.
Contribution
It introduces new asteroseismic frequencies for Altair and integrates 1D and 2D stellar models to improve age determination of a rapid rotator.
Findings
22 new oscillation frequencies identified in Altair
Age of Altair estimated at 88±10 million years
10 frequencies matched with axisymmetric modes
Abstract
Understanding the effects of rotation in stellar evolution is key to modelling early-type stars, half of which have equatorial velocities over 100 km/s. The nearby star Altair is an example of such fast-rotating stars, and furthermore, it has the privilege of being modelled by a detailed 2D concordance model that reproduces most of its observables. The aim of this paper is to include new asteroseismic frequencies to improve our knowledge of Altair, especially its age. We processed images of Altair obtained during July 2022 by the Transiting Exoplanet Survey Satellite using the halo photometry technique to obtain its light curve over this observation period. By analysing the light curve, we derived a set of 22 new frequencies in the oscillation spectrum of Altair and confirmed 12 previously known frequencies. Compared with model predictions, we could associate ten frequencies with ten…
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Taxonomy
TopicsAstronomical Observations and Instrumentation · Inertial Sensor and Navigation · Stellar, planetary, and galactic studies
