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

Hekker, S.; Ball, W. H.

doi:10.1051/0004-6361/201323121

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

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Hekker, S.
Max Planck Research Group in Stellar Ages and Galactic Evolution (SAGE), Max Planck Institute for Solar System Research, Max Planck Society;

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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.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0019-F585-4

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