Aspects of observational red giant population seismology

Дата и время публикации : 2011-09-30T10:45:00Z

Авторы публикации и институты :
Joris De Ridder

Ссылка на журнал-издание: Ссылка на журнал-издание не найдена
Коментарии к cтатье: Proc. of the workshop “Red Giants as Probes of the Structure and Evolution of the Milky Way” (Roma, 15-17 Nov 2010), Astrophysics and Space Science Proceedings, ISBN 978-3-642-18417-8 (eds. A. Miglio, J. Montalban, A. Noels). Part of RedGiantsMilkyWay/2011/ proceedings available at
Первичная категория: astro-ph.SR

Все категории : astro-ph.SR

Краткий обзор статьи: The space missions CoRoT and Kepler provide us with large samples of red giant stars wherein non-radial solar-like oscillations can be detected. This leads to the exciting opportunity to do population seismology. In this paper we give a short overview of some relevant technical aspects of the two satellites, we list and comment on some important target selection biases relevant for population seismology, and we make a case to use kernel density estimates as an alternative for histograms to characterize population characteristics

Category: Physics