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Two Dimensional Spectral Classification Using a Computer

Published online by Cambridge University Press:  12 April 2016

H. Zekl  and
I. Appenzeller
H. Zekl
Affiliation:
Landessternwarte, Künigstuhl
I. Appenzeller
Affiliation:
Landessternwarte, Künigstuhl

Abstract

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A computer program for the automatic classification of stellar spectra is described. The aim of this program is to derive accurate absolute luminosities and spectral classes of individual stars for improved spectral parallaxes. Preliminary results are presented and future applications are discussed.

Type
VI Automatic Spectral Classification
Information
International Astronomical Union Colloquium , Volume 47: Spectral Classification of the Future , 1979 , pp. 287 - 297
Copyright
Copyright © Vatican Observatory 1979

References

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Furenlid, I. (1971). Astron. Astrophys. 10, 321.Google Scholar
Wielen, R. (1975). Conference on Optical Observing Programs on Galactic Structure and Dynamics, Schmidt-Kaler, Th.; ed., Bochum, , p. 59.Google Scholar