High-resolution observations by visible and near-infrared interferometers of both single stars and binaries have made significant contributions to the foundations that underpin many aspects of our knowledge of stellar structure and evolution for cool stars. The CS16 splinter on this topic reviewed contributions of optical interferometry to date, examined highlights of current research, and identified areas for contributions with new observational constraints in the near future.
|Title of host publication||16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun|
|Subtitle of host publication||proceedings of a conference held August 28- September 2, 2010 at the University of Washington, Seattle, Washington|
|Place of Publication||Cambridge|
|Publication status||Published - 1 Dec 2011|
van Belle, G. T., Aufdenberg, J., Boyajian, T., Harper G., N. V., Hummel, C., Pedretti, E., Baines, E., White, R., Ravi, V., & Ridgway, S. (2011). Fundamental Stellar Properties from Optical Interferometry. In 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun: proceedings of a conference held August 28- September 2, 2010 at the University of Washington, Seattle, Washington (Vol. 448, pp. 517). ASP. http://adsabs.harvard.edu/abs/2011ASPC..448..517V