We are continuing a comprehensive systematic study of the properties of Wolf-Rayet Galaxies (WRGs) based on data from ground and space observatories. In this proposal we request time on the KPNO 0.9m and 2.1m telescopes to undertake CCD imagery and spectroscopy of a group of WRGs. Our basic aim is threefold: (a) identify and characterize the

Six BL Lac objects from the complete 1 Jy radio-selected sample of 34 objects were observed in cycle 5 with the Hubble Space Telescope (HST) Wide-Field Planetary Camera 2 (WFPC2) to an equivalent limiting flux of mu_I~26 mag arcsec^-2. Here we report results for the second half of this sample, as well as new results for the first three objects

We present a new high quality continuum-subtracted Hα image of NGC 7479. Using a novel semi-automated technique we have determined the positions, angular sizes, and absolute fluxes of over 1000 Hii regions and have constructed the luminosity function for the regions over the whole galaxy, showing that its slope is within the published range for

The nearly face-on spiral galaxy NGC 3938 has been observed in the H_alpha line with the TAURUS II Fabry-Perot interferometer at the William Herschel Telescope in order to study the kinematics of the ionized gas. We are able to construct intensity, velocity and velocity dispersion maps for this galaxy. The rotation curve of the galaxy is calculated

We present the results of a deep CCD-based IZ photometric survey of a ~ 1 deg(2) area in the central region of the Pleiades Galactic open cluster. The magnitude coverage of our survey (from I ~ 17.5 down to 22) allows us to detect substellar candidates with masses between 0.075 and 0.03 Msun. Details of the photometric reduction and selection

Not Available