Asteroseismology with TESS: Emergence of Dipole Mode Suppression from Subgiants?

Dipole mode suppression is an observed behavior of solar-like oscillations in evolved stars. This study aims to search for depressed dipole modes in giant stars using data from the Transiting Exoplanet Survey Satellite (TESS) and investigate when the suppression starts to emerge. We study a sample o...

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Published inThe Astrophysical journal Vol. 980; no. 2; pp. 217 - 227
Main Authors Lin, Shurui, Li, Tanda, Mao, Shude, Fuller, Jim
Format Journal Article
LanguageEnglish
Published Philadelphia The American Astronomical Society 20.02.2025
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ISSN0004-637X
1538-4357
1538-4357
DOI10.3847/1538-4357/adae9e

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Abstract Dipole mode suppression is an observed behavior of solar-like oscillations in evolved stars. This study aims to search for depressed dipole modes in giant stars using data from the Transiting Exoplanet Survey Satellite (TESS) and investigate when the suppression starts to emerge. We study a sample of 8651 evolved stars from TESS and find 179 stars with significant dipole mode depression by comparing the oscillation amplitudes of radial and dipole modes. Notably, 11 of them are located near the base of the red giant branch, indicating that mode suppression appears earlier than the point inferred in previous studies with Kepler data. These findings provide new evidence for dipole mode suppression in giant stars, particularly in subgiants.
AbstractList Dipole mode suppression is an observed behavior of solar-like oscillations in evolved stars. This study aims to search for depressed dipole modes in giant stars using data from the Transiting Exoplanet Survey Satellite (TESS) and investigate when the suppression starts to emerge. We study a sample of 8651 evolved stars from TESS and find 179 stars with significant dipole mode depression by comparing the oscillation amplitudes of radial and dipole modes. Notably, 11 of them are located near the base of the red giant branch, indicating that mode suppression appears earlier than the point inferred in previous studies with Kepler data. These findings provide new evidence for dipole mode suppression in giant stars, particularly in subgiants.
Author Lin, Shurui
Li, Tanda
Mao, Shude
Fuller, Jim
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  givenname: Shude
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  surname: Mao
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  surname: Fuller
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  organization: Walter Burke Institute for Theoretical Physics TAPIR, Caltech, Mailcode 350-17, Pasadena, CA 91125, USA
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Snippet Dipole mode suppression is an observed behavior of solar-like oscillations in evolved stars. This study aims to search for depressed dipole modes in giant...
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StartPage 217
SubjectTerms Asteroseismology
Dipoles
Extrasolar planets
Giant stars
Planet detection
Solar oscillations
Stellar evolution
Stellar magnetic fields
Stellar oscillations
Stellar seismology
Subgiant stars
Transit
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Title Asteroseismology with TESS: Emergence of Dipole Mode Suppression from Subgiants?
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