Solar-like oscillations from the depths of the red-giant star KIC 4351319 observed with Kepler
Di Mauro, M. P × Cardini, D Catanzaro, G Ventura, R Barban, C Bedding, T. R Christensen-Dalsgaard, J De Ridder, Joris Hekker, S Huber, D Kallinger, Thomas Miglio, A Montalban, J Mosser, B Stello, D Uytterhoeven, K Kinemuchi, K Kjeldsen, H Mullally, F Still, M #
Priestley and Weale
Monthly Notices of the Royal Astronomical Society vol:415 issue:4 pages:3783-3797
We present the results of the asteroseismic analysis of the red-giant star KIC 4351319 (TYC 3124-914-1), observed for 30 d in short-cadence mode with the Kepler satellite. The analysis has allowed us to determine the large and small frequency separations, Delta nu(0) = 24.6 +/- 0.2 mu Hz and Delta nu(02) = 2.2 +/- 0.3 mu Hz, respectively, and the frequency of maximum oscillation power, nu(max) = 386.5 +/- 4.0 mu Hz.