Stello, Dennis, Huber, Daniel, Kallinger, Thomas, Basu, Sarbani, Mosser, Benoît, Hekker, Saskia, Mathur, Savita, García, Rafael A., Bedding, Timothy R., Kjeldsen, Hans, Gilliland, Ronald L., Verner, Graham A., Chaplin, William J., Benomar, Othman, Meibom, Søren, Grundahl, Frank, Elsworth, Yvonne P., Molenda-Zakowicz, Joanna, Szabó, Robert, Christensen-Dalsgaard, Jørgen, Tenenbaum, Peter, Twicken, Joseph D. and Uddin, Kamal
Abstract
Scaling relations that link asteroseismic quantities to global stellar properties are important for gaining understanding of the intricate physics that underpins stellar pulsations. The common notion that all stars in an open cluster have essentially the same distance, age, and initial composition implies that the stellar parameters can be measured
