Global Asteroseismic Parameters of NGC 6791 and NGC6819
1 : The University of Sydney
(USYD)
Physics Office, Room 210, Building A28 SIfA, H90 School of Physics University of Sydney NSW 2006 Australia -
Australia
We present preliminary results of an asteroseismic analysis of the open clusters NGC 6791 and NGC 6819 in the Kepler field of view. We analysed 103 stars to extract the asteroseismic properties max and to make them available to the scientific community. We used a simple stitching algorithm to correct for the jumps in the Kepler light curves between each quarter. We use the SYD pipeline to measure the asteroseismic values and compared these values to the expected values for cluster membership to find new member stars for each cluster. We also provide a comparison of previous membership studies.