Red Clump stars in Kepler open cluster NGC 6819

We measure the large frequency separation, Δν, and the frequency of maximum amplitude, νmax, for 10 Red Clump (RC) single member (SM) stars in the Kepler open cluster NGC 6819. We derive luminosities and masses for each individual RC star. A comparison of the observations with an isochrone of Age =...

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Библиографические подробности
Главные авторы: Abedigamba O.P., Balona L.A., Medupe T.R.
Формат: Статья
Язык:English
Опубликовано: EDP Sciences 2015-01-01
Серии:EPJ Web of Conferences
Online-ссылка:http://dx.doi.org/10.1051/epjconf/201510106001