Applications of Fourier analysis to broadening of stellar line profiles. IV - A technique for separating macroturbulence from rotation in solar-type stars

Details Applications of Fourier analysis to broadening of stellar line profiles. IV - A technique for separating macroturbulence from rotation in solar-type stars Applications of Fourier analysis to broadening of stellar line profiles. IV - A technique for separating macroturbulence from rotation in solar-type stars

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...208..487s&link_type=abstract

Astrophysical Journal, vol. 208, Sept. 1, 1976, pt. 1, p. 487-499.

Astronomy and Astrophysics

Astrophysics

28

Fourier Transformation, Spectral Line Width, Stellar Rotation, Stellar Spectra, Chromosphere, Error Analysis, Signal To Noise Ratios, Solar Rotation, Turbulence Effects, Turbulent Flow, Velocity Distribution

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1976ApJ...208..487S

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