En este trabajo se presenta un conjunto de datos espectroscópicos obtenidos de una muestra de galaxias de diferentes tipos morfológicos. Estos datos se discuten con la intención de analizar comparativamente la cinemática del gas y de las estrellas. Los resultados son muy heterogéneos pero conducen a una conclusión fundamental la cinemática del gas

Based on ISO SWS+LWS observations, we identify IRAS 16594-4656 as a new member of the rare class of C-rich proto-planetary nebulae with the 21 μm dust feature in emission. In addition, the major PAHs emission bands at 3.3, 6.2, 7.7, 8.6 and 11.3 μm are detected, together with unusually strong features at 12.6 and 13.4 μm , very rarely observed

Geochemical study of lunar meteorite EET96008 shows that it is a heterogeneous basaltic breccia containing matrix and clasts of variable composition. Comparison with EET87521 shows that the two breccias are almost certainly paired meteorites.

Narrowband images of 51 symbiotic stars were obtained at the ESO and ORM observatories to search for resolved optical nebulae. Ionized nebulae much larger than previously known are found around CH Cyg, HM Sge and V1016 Cyg, and they will be discussed in detail in forthcoming papers. A nebula with a deconvolved size between 0farcs9 and 1farcs5 is

IAUC 7113 available at Central Bureau for Astronomical Telegrams.

We present two-dimensional optical spectroscopy of the central region (9.4"x12.2") of the Seyfert 1 ring galaxy NGC 985 obtained with an optical fiber system (two-dimensional Fiber ISIS System). The 95 spectra presented here include the Hβ-[O III] lambdalambda4959, 5007 emission lines and the Mg I b absorption lines, which permit the study of the