Résumé
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.
| langue originale | English |
|---|---|
| titre | 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun |
| Sous-titre | proceedings of a conference held August 28- September 2, 2010 at the University of Washington, Seattle, Washington |
| Lieu de publication | Cambridge |
| Editeur | ASP |
| Pages | 517 |
| Volume | 448 |
| état | Published - 1 déc. 2011 |
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