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Detectability of Bulge stars

Published online by Cambridge University Press:  07 August 2017

M. Hernandez-Pajares
Affiliation:
Departament de Matemàtica Aplicada i Telemàtica
R. Cubarsi
Affiliation:
Departament de Matemàtica Aplicada i Telemàtica
J. Sanz-Subirana
Affiliation:
Departament de Matemàtica Aplicada i Telemàtica
J.M. Juan-Zornoza
Affiliation:
Departament de Física Aplicada ETSETB, Universitat Politècnica de Catalunya, P. O. Box 30002, E-08080 Barcelona, Spain First author's e-mail: [email protected]

Abstract

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Classification algorithms based on neural network techniques are applied to study if the bulge stars can be differentiated from other stars belonging to other Galactic components. A synthetic sample is build as a mixture of four components, thin disk, thick disk, halo and bulge, according to some stellar system models and considering observational errors.

Type
Contributed Papers
Copyright
Copyright © Kluwer 1993 

References

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