Abstract
We investigate properties of the internal structure of HR2021, better known as β Hydri, a G2 IV subgiant with mass close to solar and for which observations by Bedding et al. (2001) have shown the presence of solar-like oscillations. We have computed models of β Hydri, based on updated global parameters, and compared the computed frequencies for the models with the observed oscillation spectrum.
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© 2003 Springer Science+Business Media Dordrecht
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Mauro, M.P.D., Christensen-Dalsgaard, J., Paternò, L. (2003). A Study of the Solar-Like Properties of β Hydri. In: Thompson, M.J., Cunha, M.S., Monteiro, M.J.P.F.G. (eds) Asteroseismology Across the HR Diagram. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-0799-2_30
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DOI: https://doi.org/10.1007/978-94-017-0799-2_30
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-6241-3
Online ISBN: 978-94-017-0799-2
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