The peculiar galaxy NGC 520 (Arp 157) is often interpreted as an interacting pair of galaxies. The identification of the two bulges and overall morphology of the two galaxies has long been a puzzle which the authors attempt to solve here. New longslit optical spectroscopy and near-infrared images of NGC 520 are presented. These data suggest that

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IAUC 5131 available at Central Bureau for Astronomical Telegrams. IAUC 5131 available at Central Bureau for Astronomical Telegrams.

RESUMEN. Presentamos observaciones de la estrella HD 213534 (GX Peg) efectuadas dentro de una campafia para determinar los limites de detecciotn e tierra de oscilaciones de alta frecuencia y pequena amplitud. ABSTRACT. Observations of the star HD 213534 (GX Peg) made to determine the detection limits for high frequency and small amplitude star

. Medjante fotometria fotoelectrica BV fueron estudiados 31 EUPHROSYNE, 118 PEITHO en su oposici6n de 1988, y 13 EGERIA, 196 PHILOMENA y 471 PAPAGENA en su oposici6n de 1989, con el fin de determinar su per1odo de rotaci6n, la orientaci6n del polo y la forma de los asteroides. Se presentan las curvas de luz de 118 PEITHO y 13 EGERIA. ABSTRACT. The

The authors obtained near infrared images in J, H, and K filters of the H II region N159 in the LMC with the IR Imager on the 1.5 m telescope of CTIO. Some 50 sources are detected in an area of roughly 10 arc min squared. The region seems to be a site of active star formation associated to a large molecular complex and possibly coincides with one