Volume 620, December 2018
|Number of page(s)||1|
|Section||Stellar structure and evolution|
|Published online||17 December 2018|
Absolute parameters for AI Phoenicis using WASP photometry (Corrigendum)
Astrophysics Group, Keele University, Keele, Staffordshire ST5 5BG, UK
2 Institute of Space Sciences (ICE, CSIC) Campus UAB, Carrer de Can Magrans, s/n, 08193 Barcelona, Spain
3 Institut d’Estudis Espacials de Catalunya (IEEC), C/Gran Capita, 2-4, 08034 Barcelona, Spain
4 Department of Physics, University of Warwick, Coventry, CV4 7AL, UK
Key words: stars: solar-type / stars: evolution / stars: fundamental parameters / binaries: eclipsing / errata / addenda
An error has been noted in the linear ephemeris for AI Phe, shown in Eq. (2) of the paper. The correct ephemeris is
This is typographical error and has no effect on any of the timing analysis presented in the paper.
© ESO 2018
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.