摘要
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.
| 源语言 | English |
|---|---|
| 主期刊名 | 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun |
| 主期刊副标题 | proceedings of a conference held August 28- September 2, 2010 at the University of Washington, Seattle, Washington |
| 出版地点 | Cambridge |
| 出版商 | ASP |
| 页 | 517 |
| 卷 | 448 |
| 出版状态 | Published - 1 12月 2011 |
指纹
探究 'Fundamental Stellar Properties from Optical Interferometry' 的科研主题。它们共同构成独一无二的指纹。引用此
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