Volume 607, November 2017
|Number of page(s)||1|
|Section||Stellar structure and evolution|
|Published online||17 November 2017|
Period spacings in red giants (Corrigendum)
III. Coupling factors of mixed modes⋆
1 LESIA, Observatoire de Paris, PSL Research University, CNRS, Université Pierre et Marie Curie, Université Paris Diderot, 92195 Meudon, France cedex, France
2 Department of Astronomy, School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, 113-0033 Tokyo, Japan
3 Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, 4150-762 Porto, Portugal
Key words: stars: oscillations / stars: interiors / stars: evolution / errata, addenda
A table is only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (126.96.36.199) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/600/A1
A table with the coupling factors and their uncertainties, computed as in Sect. 3 of the original paper, has been appended to the article as a CDS/VizieR document. This table downloadable at http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/600/A1 contains 5166 stars identified with their KIC numbers, coordinates, large separations Δν, period spacings ΔΠ1, and seismic estimates of the mass.
© ESO, 2017
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.