At less than 4 Mpc away, Centaurus A (NGC 5128) is the nearest massive elliptical galaxy, the nearest radio galaxy, and the nearest recent merger. It is the...
The Nucleus-Host Galaxy Connection in Radio-Loud AGN
We studied a moderate-redshift (0.15 5 orders of magnitude in nuclear power, and the two sub-samples have indistinguishable luminosity--redshift distributions...
The O III narrow line shapes in spectra of Mrk 817.
The O III (4959, 5007) lines from spectra of Mrk 817 obtained from a 9-year long period were analyzed. A blue asymmetry of the lines is noticeable. The authors...
The VLT-FLAMES Tarantula Survey (VFTS) has secured mid-resolution spectra of over 300 O-type stars in the 30 Doradus region of the Large Magellanic Cloud. A...
The Tarantula FLAMES Survey is an ESO Large Program aimed at disentangling the role of binarity in the evolution of massive stars. We have multiepoch, high...
LINERs have been a class of low-luminosity AGN difficult to explain under the unified model. It has been claimed (González-Martín et al. 2009b) that a high...
The Observatorio Astrofísico de Javalambre: current status, developments, operations, and strategies
The Observatorio Astrofísico de Javalambre (OAJ) is a new Spanish astronomical facility particularly designed for carrying out large sky surveys. The OAJ is...
The Observatorio Astrofísico de Javalambre: goals and current status
The Observatorio Astrofsico de Javalambre in Spain is a new astronomical facility particularly conceived for carrying out large sky surveys with two...
The Observatorio del Teide welcomes SONG:the Stellar Observations Network Group
The Stellar Observations Network Group (SONG) is an internationalnetwork project aiming to place eight 1 m robotic telescopes around the globe,with the primary...