The Astrophysical Journal (Jan 2024)

Asteroseismology of the Nearby K Dwarf σ Draconis Using the Keck Planet Finder and TESS

  • Marc Hon,
  • Daniel Huber,
  • Yaguang Li,
  • Travis S. Metcalfe,
  • Timothy R. Bedding,
  • Joel Ong,
  • Ashley Chontos,
  • Ryan Rubenzahl,
  • Samuel Halverson,
  • Rafael A. García,
  • Hans Kjeldsen,
  • Dennis Stello,
  • Daniel R. Hey,
  • Tiago Campante,
  • Andrew W. Howard,
  • Steven R. Gibson,
  • Kodi Rider,
  • Arpita Roy,
  • Ashley D. Baker,
  • Jerry Edelstein,
  • Chris Smith,
  • Benjamin J. Fulton,
  • Josh Walawender,
  • Max Brodheim,
  • Matt Brown,
  • Dwight Chan,
  • Fei Dai,
  • William Deich,
  • Colby Gottschalk,
  • Jason Grillo,
  • Dave Hale,
  • Grant M. Hill,
  • Bradford Holden,
  • Aaron Householder,
  • Howard Isaacson,
  • Yuzo Ishikawa,
  • Sharon R. Jelinsky,
  • Marc Kassis,
  • Stephen Kaye,
  • Russ Laher,
  • Kyle Lanclos,
  • Chien-Hsiu Lee,
  • Scott Lilley,
  • Ben McCarney,
  • Timothy N. Miller,
  • Joel Payne,
  • Erik A. Petigura,
  • Claire Poppett,
  • Michael Raffanti,
  • Constance Rockosi,
  • Dale Sanford,
  • Christian Schwab,
  • Abby P. Shaum,
  • Martin M. Sirk,
  • Roger Smith,
  • Jim Thorne,
  • John Valliant,
  • Adam Vandenberg,
  • Shin Ywan Wang,
  • Edward Wishnow,
  • Truman Wold,
  • Sherry Yeh,
  • Ashley Baker,
  • Sarbani Basu,
  • Megan Bedell,
  • Heather M. Cegla,
  • Ian Crossfield,
  • Courtney Dressing,
  • Xavier Dumusque,
  • Heather Knutson,
  • Dimitri Mawet,
  • John O’Meara,
  • Guđmundur Stefánsson,
  • Johanna Teske,
  • Gautam Vasisht,
  • Sharon Xuesong Wang,
  • Lauren M. Weiss,
  • Joshua N. Winn,
  • Jason T. Wright

DOI
https://doi.org/10.3847/1538-4357/ad76a9
Journal volume & issue
Vol. 975, no. 1
p. 147

Abstract

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Asteroseismology of dwarf stars cooler than the Sun is very challenging owing to the low amplitudes and rapid timescales of oscillations. Here we present the asteroseismic detection of solar-like oscillations at 4-minute timescales ( ${\nu }_{\max }\sim 4300$ μ Hz) in the nearby K dwarf σ Draconis using extreme-precision Doppler velocity observations from the Keck Planet Finder and 20 s cadence photometry from NASA’s Transiting Exoplanet Survey Satellite. The star is the coolest dwarf star to date with both velocity and luminosity observations of solar-like oscillations, having amplitudes of 5.9 ± 0.8 cm s ^−1 and 0.8 ± 0.2 ppm, respectively. These measured values are in excellent agreement with established luminosity−velocity amplitude relations for oscillations and provide further evidence that mode amplitudes for stars with T _eff < 5500 K diminish in scale following an ( L / M ) ^1.5 relation. By modeling the star’s oscillation frequencies from photometric data, we measure an asteroseismic age of 4.5 ± 0.9 (ran) ± 1.2 (sys) Gyr. The observations demonstrate the capability of next-generation spectrographs and precise space-based photometry to extend observational asteroseismology to nearby cool dwarfs, which are benchmarks for stellar astrophysics and prime targets for directly imaging planets using future space-based telescopes.

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