NASA NTRS · 19800016749
Microturbulence and Wesselink radii
Abstract
Using the calibration of Bell and Parsons (1974), the effects of changes in microturbulence and surface gravity throughout the cycles of delta Cephei and eta Aquilae are estimated. When the changes in microturbulence are considered, Wesselink radii for these stars are reduced 20%.
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Evans, N. R.. 1980-05-01. Microturbulence and Wesselink radii. https://ntrs.nasa.gov/citations/19800016749
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