Fundamental Stellar Properties from Optical Interferometry
Solar and Stellar Astrophysics
2015-03-17 v1 Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
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.
Cite
@article{arxiv.1012.1146,
title = {Fundamental Stellar Properties from Optical Interferometry},
author = {Gerard T. van Belle and Jason Aufdenberg and Tabetha Boyajian and Graham Harper and Christian Hummel and Ettore Pedretti and Ellyn Baines and Russel White and Vikram Ravi and Steve Ridgway},
journal= {arXiv preprint arXiv:1012.1146},
year = {2015}
}
Comments
Contribution to Proceedings of Cool Stars 16 Workshop; 14 pages in ASP format; 4 figures