Predicting accurate stellar angular diameters by the near-infrared surface brightness technique
- 6 January 2005
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 357 (1) , 174-190
- https://doi.org/10.1111/j.1365-2966.2005.08632.x
Abstract
No abstract availableKeywords
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