Abstract
We present the application of the Learning Vectorial Quantification Neural Method to the study of a stellar catalogue containing more than 12000 stars. One of the first results is the appearance of three statistically well defined groups of stars that fulfill some kinematic properties corresponding to the Thin Disk, Thick Disk and Halo components of the Milky Way.
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© 1991 Springer-Verlag Berlin Heidelberg
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Hernandez-Pajares, M., Monte, E. (1991). Application of the LVQ neural method to a stellar catalogue. In: Prieto, A. (eds) Artificial Neural Networks. IWANN 1991. Lecture Notes in Computer Science, vol 540. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0035923
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DOI: https://doi.org/10.1007/BFb0035923
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