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  Scaling Relations for Solar-Like Oscillations: A Review

Hekker, S. (2020). Scaling Relations for Solar-Like Oscillations: A Review. Frontiers in Astronomy and Space Sciences, 7: 3. doi:10.3389/fspas.2020.00003.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0006-A02B-5 Version Permalink: http://hdl.handle.net/21.11116/0000-0006-A02C-4
Genre: Journal Article

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 Creators:
Hekker, Saskia1, Author              
Affiliations:
1Max Planck Research Group in Stellar Ages and Galactic Evolution (SAGE), Max Planck Institute for Solar System Research, Max Planck Society, ou_2265636              

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 Abstract: The scaling relations for solar-like oscillations provide a translation of the features of the stochastic low-degree modes of oscillation in the Sun to predict the features of solar-like oscillations in other stars with convective outer layers. This prediction is based on their stellar mass, radius, and effective temperature. Over time, the original scaling relations have been reversed in their use from predicting features of solar-like oscillations to deriving stellar parameters. Updates to the scaling relations as well as their reference values have been proposed to accommodate for the different requirements set by the change in their use. In this review the suggestions for improving the accuracy of the estimates of stellar parameters through the scaling relations for solar-like oscillations are presented together with a discussion of pros and cons of different approaches.

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Language(s): eng - English
 Dates: 2020
 Publication Status: Published in print
 Pages: -
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 Table of Contents: -
 Rev. Method: Peer
 Identifiers: DOI: 10.3389/fspas.2020.00003
 Degree: -

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Title: Frontiers in Astronomy and Space Sciences
Source Genre: Journal
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Publ. Info: Lausanne : Frontiers Media
Pages: - Volume / Issue: 7 Sequence Number: 3 Start / End Page: - Identifier: ISSN: 2296-987X
CoNE: https://pure.mpg.de/cone/journals/resource/2296-987X