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Globular Clusters as Candidates for Gravitational Lenses to Explain Quasar-Galaxy Associations
We argue that globular clusters (GCs) are good candidates forgravitational lenses in explaining quasar-galaxy associations. Thecatalog of associations (Bukhmastova 2001) compiled from the LEDAcatalog of galaxies (Paturel 1997) and from the catalog of quasars(Veron-Cetty and Veron 1998) is used. Based on the new catalog, we showthat one might expect an increased number of GCs around irregulargalaxies of types 9 and 10 from the hypothesis that distant compactsources are gravitationally lensed by GCs in the halos of foregroundgalaxies. The King model is used to determine the central surfacedensities of 135 GCs in the Milky Way. The distribution of GCs incentral surface density was found to be lognormal.

Total magnitude, radius, colour indices, colour gradients and photometric type of galaxies
We present a catalogue of aperture photometry of galaxies, in UBVRI,assembled from three different origins: (i) an update of the catalogueof Buta et al. (1995) (ii) published photometric profiles and (iii)aperture photometry performed on CCD images. We explored different setsof growth curves to fit these data: (i) The Sersic law, (ii) The net ofgrowth curves used for the preparation of the RC3 and (iii) A linearinterpolation between the de Vaucouleurs (r(1/4) ) and exponential laws.Finally we adopted the latter solution. Fitting these growth curves, wederive (1) the total magnitude, (2) the effective radius, (3) the colourindices and (4) gradients and (5) the photometric type of 5169 galaxies.The photometric type is defined to statistically match the revisedmorphologic type and parametrizes the shape of the growth curve. It iscoded from -9, for very concentrated galaxies, to +10, for diffusegalaxies. Based in part on observations collected at the Haute-ProvenceObservatory.

The statistics analysis of recent supernovae.
Not Available

The molecular gas content of spiral galaxies in compact groups.
We present ^12^CO(J=1-0) line observations of 15 late-type opticallyselected galaxies in compact groups. In order to study the effects ofenvironment on the molecular content of compact group galaxies we usethe CO(1-0) emission to estimate an indicative molecular hydrogencontent of the target galaxies adopting a standard conversion factorX=N(H_2_)/I(CO). We compare the frequency distribution of the normalizedhybrid molecular gas surface density to the one obtained for anoptically selected reference sample of isolated galaxies. Despite theirhigh-density environment, compact group galaxies have, on average,similar CO emission compared to isolated galaxies of same sizes andluminosities. However there are some compact group galaxies withperturbed morphologies and high far-infrared fluxes which have anenhanced CO emissivity.

Supernova 1994Z in NGC 87
IAUC 6087 available at Central Bureau for Astronomical Telegrams.

Southern Galaxy Catalogue.
Not Available

Faint stellar spectral-type standards for objective-prism plates from the UK 1.2-m Schmidt
Illustrations and descriptions are given for 10 stellar spectral typesfrom A3 to M5 as they appear on photographs obtained with the objectiveprism of the UK Schmidt telescope. The corresponding slit spectra at18-A resolution also are shown from the image photon-counting system ofthe 3.9-m Anglo-Australian telescope. The stars range betweenmB = 14.8 and 18.8 with little or no reddening.

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Observation and Astrometry data

Right ascension:00h21m14.00s
Aparent dimensions:0.871′ × 0.724′

Catalogs and designations:
Proper Names   (Edit)
NGC 2000.0NGC 87

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