Published December 6, 2010 | Version Submitted
Discussion Paper Open

Fundamental Stellar Properties from Optical Interferometry

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.

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Submitted - 1012.1146.pdf

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1012.1146.pdf

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Additional details

Identifiers

Eprint ID
96889
DOI
10.48550/arXiv.1012.1146
Resolver ID
CaltechAUTHORS:20190702-135001947

Related works

Funding

NASA Hubble Fellowship

Dates

Created
2019-07-08
Created from EPrint's datestamp field
Updated
2023-06-02
Created from EPrint's last_modified field