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Effective temperatures

Temperatures of stars are derived from their spectral type and luminosity class. Calibrations are stored in files spec_par.V, spec_par.IV, spec_par.III, spec_par.II, spec_par.I in oyster/starbase.

teff_stars Compute effective temperature for all stars in startable.

Function. Return effective temperature for star with specified spectrum.

Christian Hummel 2017-06-29