Atmospheric turbulence measured in stars above the main sequence

Details Atmospheric turbulence measured in stars above the main sequence Atmospheric turbulence measured in stars above the main sequence

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...202..148g&link_type=abstract

Astrophysical Journal, vol. 202, Nov. 15, 1975, pt. 1, p. 148-164. Research supported by the National Research Council of Canad

Astronomy and Astrophysics

Astrophysics

73

Atmospheric Turbulence, Line Spectra, Stellar Atmospheres, Stellar Rotation, Giant Stars, Spectral Line Width, Supergiant Stars, Velocity Distribution

Scientific paper

Measurements of broadened line profiles are analyzed to identify,
measure, and separate macroturbulence from rotation. Evidence is
presented for the possibility of more than one macroturbulence velocity
distribution.

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