Microturbulence and Wesselink radii

Details Microturbulence and Wesselink radii Microturbulence and Wesselink radii

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980cpsp.book..237e&link_type=abstract

In NASA. Goddard Space Flight Center Current Probl. in Stellar Pulsation Instabilities p 237-246 (SEE N80-25229 15-90)

Physics

8

Gas Dynamics, Low Level Turbulence, Radial Velocity, Stellar Gravitation, Stellar Mass, Variable Stars, Brightness, Color, Pulse Amplitude, Spectral Line Width, Stellar Spectra

Scientific paper

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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