M. P. Di Mauro, D. Cardini, R. Ventura, D. Stello, P. G. Beck, G. Davies, Y. Elsworth, R. A. Garcıa, S. Hekker, B. Mosser, J. Christensen-Dalsgaard, S. Bloemen, G. Catanzaro, K. De Smedt, A. Tkachenko
Published 2012-12-19Version 1
We present an asteroseismic approach to study the dynamics of the stellar interior in red-giant stars by asteroseismic inversion of the splittings induced by the stellar rotation on the oscillation frequencies. We show preliminary results obtained for the red giant KIC4448777 observed by the space mission Kepler.
Comments: 3 pages, 4 figures, the 40th Liege International Astrophysical Colloquium Liac40, 'Ageing low mass stars: from red giants to white dwarfs', to be published on EPJ Web of Conferences
Internal rotation of the red-giant star KIC 4448777 by means of asteroseismic inversion
Asteroseismology of 19 low-luminosity red giant stars from Kepler
Asteroseismology: Data Analysis Methods and Interpretation for Space and Ground-based Facilities
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