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The luminosity class introduced by Van den Bergh (1960) has been numerically coded between 1 and 9 with the extension introduced by H.G. Corwin (SGC, 1985) between 9 and 11. The luminosity class is coded on a continuous scale which is related to the original classification as: . The original nomenclature was chosen to match the Yerkes system of stellar luminosities. HyperLeda . Questions: prugniel@obs.univ-lyon1.fr

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