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Solar-Like Oscillations in β Hydri: Evidence for Short-Lived High-Amplitude Oscillations

Published online by Cambridge University Press:  12 April 2016

T.R. Bedding
Affiliation:
School of PhysicsA28, University of Sydney, NSW 2006, Australia
H. Kjeldsen
Affiliation:
Theoretical Astrophysics Center, University of Aarhus, Denmark
I.K. Baldry
Affiliation:
Anglo-Australian Observatory, Epping, Australia
F. Bouchy
Affiliation:
Observatoire de Genève, Sauverny, Switzerland
R.P. Butler
Affiliation:
Carnegie Institution of Washington, Washington, DC, USA
F. Carrier
Affiliation:
Observatoire de Genève, Sauverny, Switzerland
F. Kienzle
Affiliation:
Observatoire de Genève, Sauverny, Switzerland
G.W. Marcy
Affiliation:
Department of Astronomy, University of California, Berkeley, CA
S.J. O’Toole
Affiliation:
School of PhysicsA28, University of Sydney, NSW 2006, Australia
C.G. Tinney
Affiliation:
Anglo-Australian Observatory, Epping, Australia

Abstract

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Velocity measurements of the G2 subgiant β Hyi with both UCLES and CORALIE show a clear excess of power centred at 1.0 mHz. In the UCLES data we find evidence for a short-lived, high-amplitude oscillation event. If confirmed as a feature of subgiants, such ‘starquakes’ would make it harder to measure accurate mode frequencies and perform asteroseismology.

Type
Part 4. The Interaction between Convection and Pulsation
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Bedding, T.R., Butler, R.P., Kjeldsen, H., et. al. 2001, ApJ, 549, L105 CrossRefGoogle Scholar
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