We present a new method based on artificial neural networks trained with multiseed backpropagation, for displaying an n-dimensional distribution in a projected space of one, two, or three dimensions. As principal component analysis (PCA) the proposed method is useful for extracting information on the structure of the data set, but unlike the PCA

ISOPHOT is one of four instruments onboard the ESA Infrared Space Observatory scheduled for launch in September 1995. It covers the wavelength range 2.5 micrometers to 240 micrometers with wide and marrow spectral bands. Diffraction limited observations as well as wide beam measurements of faint extended sources are possible. Polarimetric

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IAUC 5879 available at Central Bureau for Astronomical Telegrams. IAUC 5879 available at Central Bureau for Astronomical Telegrams.

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SE REALIZA UN ANALISIS CINEMATICO Y MORFOLOGICO DE CUATRO NEBULOSAS PLANETARIAS DE TIPO I BIPOLARES, ADEMAS DEL ESTUDIO ESPACIAL DE PARAMETROS FISICO-QUIMICOS. SE HAN DESARROLLADO HERRAMIENTAS DE CALCULO QUE PERMITEN ELABORAR MODELOS CINEMATICOS Y MORFOLOGICOS: CONSTRUCCION DE MAPAS DE VELOCIDADES, DESARROLLO DE MODELOS DE ONDAS DE CHOQUE