The results of an intensive site testing assessment campaign, held at the Observatorio del Roque de los Muchachos (ORM) (La Palma) during four nights on July 1990 are presented and discussed. To evaluate the optical quality of an astronomical site for high angular resolution astronomy our philosophy leads us to make use of as many instruments as

EL OBJETIVO DE ESTE TRABAJO ES EL ESTUDIO DE BLAZANES Y DE QUASARES EN GENERAL, CON LA INTENCION DE ESTABLECER LAS POSIBLES SIMILITUDES Y DIFERENCIAS QUE PUEDAN CLARIFICAR LA CLASIFICACION DE ESTOS OBJETOS. CON ESTA IDEA SE HA DESARROLLADO UN IMPORTANTE PROGRAMA OBSERVACIONAL EN EL VISIBLE E INFRARROJO ESTUDIANDO LA VARIABILIDAD DE ESTOS OBJETOS

Results of a five-month campaign of optical monitoring the Seyfert 1 galaxy NGC 4593 are presented. High resolution H-alpha and H-Beta spectra and direct images in the Johnson U, B, V, R, and I bands were obtained between January and June 1990. The emission lines and the continuum showed strong variations on time scales of weeks to days. The H

We present lightcurves ofasteroids 31 Euphrosyne, 196 Philomena and 471 Papagena and apply two different amplitude-aspect methods for pole and shape determination.

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