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  Grid-based seismic modelling at high and low signal-to-noise ratios. HD 181420 and HD 175272

Hekker, S., & Ball, W. H. (2014). Grid-based seismic modelling at high and low signal-to-noise ratios. HD 181420 and HD 175272. Astronomy and Astrophysics, 564: A105. doi:10.1051/0004-6361/201323121.

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 Creators:
Hekker, S.1, Author              
Ball, W. H., Author
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1Max Planck Research Group in Stellar Ages and Galactic Evolution (SAGE), Max Planck Institute for Solar System Research, Max Planck Society, Justus-von-Liebig-Weg 3, 37077 Göttingen, DE, ou_2265636              

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 MPIS_PROJECTS: StellarAges
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 Dates: 2014
 Publication Status: Published in print
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 Rev. Type: Peer
 Identifiers: DOI: 10.1051/0004-6361/201323121
BibTex Citekey: Hekker:2014-045
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Title: Astronomy and Astrophysics
Source Genre: Journal
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Pages: - Volume / Issue: 564 Sequence Number: A105 Start / End Page: - Identifier: -