Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.eso.org/~chummel/oyster/manual/node116.html
Дата изменения: Tue Apr 28 19:12:50 2015
Дата индексирования: Sun Apr 10 20:37:29 2016
Кодировка:
Поисковые слова: mercury surface
Effective temperatures next up previous contents
Next: Diameters Up: Stellar parameters from calibrations Previous: Gravities   Contents

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.
teff_star(spectrum$<$_char$>$)

Function. Return effective temperature for star with specified spectrum.


Christian Hummel 2015-04-28