Aims: Exo-planets are preferentially found around high metallicity main sequence stars. We investigate whether evolved stars share this property, and its implications for planet formation. Methods: Statistical tools and the basic concepts of stellar evolution theory are applied to published results as well as our own radial velocity and chemical

The optical properties of a number of supercompact ultraviolet luminous galaxies (UVLGs), recently discovered in the local universe matching Galaxy Evolution Explorer (GALEX) and Sloan Digital Sky Survey (SDSS) data, are discussed. Detailed reanalysis of the SDSS data for these and other similar but nearer galaxies shows that their surface

I take a critical look at the way in which electronic publishing has changed the world of publishing beyond recognition over the past decade. While the e-publishing revolution has brought many benefits to academic and research communication, there are a number of factors that inhibit the flow of information. I argue that a new publishing culture is

Accretion onto a black hole (BH) is the most viable explanation for the huge emitted power in active galaxies. A wealth of observations have shown the presence of a BH in many nearby inactive bulges, suggesting that all massive spheroids harbor a BH. At low redshift, fundamental correlations have been found between the BH mass and the luminosity

Recently, it has been showed that (136108) 2003 EL61 and its biggest satellite S/2005 (136108) 1,(55636) 2002 TX300, (13308) 1996 TO66 , OP32, 1995 SM55 and 2005 RR43 are part of a population trans-netunian objects (TNOs) clustered in the space of orbital parameters (41.6

In order to characterized the vertical atmospheric structure at the Teide Observatory (Tenerife, Spain), we are using two different remote sensing technics: SODAR (SOund Detection And Ranging) and SCIDAR (SCIncitillation Detection And Ranging) at this astronomical site. We present in this work the preliminar results on the comparison of the