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Low Dispersion Spectrophotometry of Late Type Stars

Published online by Cambridge University Press:  14 August 2015

H. Moreno
H. Moreno*
Affiliation:
Departamento de Astronomía, Universidad de Chile

Abstract

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Low dispersion (slit 60 Å wide) spectrophotometric observations of late type stars have been made. The sample of stars observed cover from K0 to M8 and luminosity classes V to I.

A selection of these stars including each luminosity class and spectral type is being analyzed. The observed intensity distributions have been corrected for atmospheric extinction and have been normalized to a common maximum intensity. The resulting instrumental intensity distributions are being studied for the best parameters for spectral classification.

Information

Type
Part III: Photometric Classification
Information
Symposium - International Astronomical Union , Volume 50: Spectral Classification and Multicolour Photometry , 1973 , pp. 267 - 271
Copyright
Copyright © Reidel 1973 

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