文章基本信息

标题：Oscillation mode linewidths and heights of 23 main-sequence stars observed by Kepler (Corrigendum)
本地全文：下载
作者：T. Appourchaux ; T. Appourchaux ; H. M. Antia 等
期刊名称：Astronomy & Astrophysics
印刷版ISSN：0004-6361
电子版ISSN：1432-0746
出版年度：2016
卷号：595
页码：1-3
DOI：10.1051/0004-6361/201323317e
语种：English
出版社：EDP Sciences
摘要：In Appourchaux et al. (2014), the correct Eq. (1) should have been written with a minus sign in front of the second bracket as ln(Γ) = (αln(ν/ν max ) + lnΓ α ) −    ln∆Γ dip 1 + ? 2ln(ν/ν dip ) ln(W dip /ν max ) ? 2    , (1) where ν is the mode frequency, ν max is the frequency of max- imum mode height, α is the power law index, Γ α is the fac- tor of the power law, ∆Γ dip is the depth of the dip, W dip is the width of the dip and ν dip is the frequency of the dip. The fits in Appourchaux et al. (2014) were indeed performed with the mi- nus sign.
关键词：stars: interiors;asteroseismology;methods: data analysis;errata, addenda