Fundamental Stellar Properties from Optical Interferometry

G. T. van Belle, J. Aufdenberg, T. Boyajian, [No Value] Harper G., C. Hummel, E. Pedretti, E. Baines, R. White, V. Ravi, S. Ridgway

Research output: Chapter in Book/Report/Conference proceedingConference contribution


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.
Original languageEnglish
Title of host publication16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
Subtitle of host publicationproceedings of a conference held August 28- September 2, 2010 at the University of Washington, Seattle, Washington
Place of PublicationCambridge
Publication statusPublished - 1 Dec 2011


Dive into the research topics of 'Fundamental Stellar Properties from Optical Interferometry'. Together they form a unique fingerprint.

Cite this