Published December 6, 2010
| Submitted
Discussion Paper
Open
Fundamental Stellar Properties from Optical Interferometry
Chicago
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Abstract
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.
Additional Information
The splinter organizers would like to thank the splinter organizing committee (Rachel Akeson, Jason Aufdenberg, Andrew Boden, Tabetha Boyajian, Michelle Creech-Eakman, Christian Hummel, Stephen Ridgway, Peter Tuthill, GvB) for their contributions to the development of the splinter program, and to the organizers of CS16 for providing the splinter opportunity.Attached Files
Submitted - 1012.1146.pdf
Files
1012.1146.pdf
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Additional details
- Eprint ID
- 96889
- DOI
- 10.48550/arXiv.1012.1146
- Resolver ID
- CaltechAUTHORS:20190702-135001947
- NASA Hubble Fellowship
- Created
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2019-07-08Created from EPrint's datestamp field
- Updated
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2023-06-02Created from EPrint's last_modified field