In a recent book, Dodson (2009) has presented an updated impression of the Amarna period, in heavy contrast to the one lately defended by Krauss (2008) and...
Do AGN triggering mechanisms vary with radio power? - I. Optical morphologies of radio-intermediate HERGs
Active galactic nuclei (AGNs) with intermediate radio powers are capable of driving multiphase outflows in galaxy bulges, and are also more common than their...
Do AGN triggering mechanisms vary with radio power? - II. The importance of mergers as a function of radio power and optical luminosity
Investigation of the triggering mechanisms of radio active galactic nuclei (radio AGN) is important for improving our general understanding of galaxy evolution...
Do all bright elliptical galaxies have active nuclei?
The evidence is noted that (1) a flux density limited complete sample of X-ray emitting BL Lac type sources is now available from Schwartz and Ku (1983), that...
We present deep near-infrared Ks -band Anglo-Australian Telescope Infrared Imager and Spectrograph observations of a selected sample of nearby barred spiral...
Do evolved stars in the LMC show dual dust chemistry?
We study a group of evolved M-stars in the Large Magellanic Cloud, characterized by a peculiar spectral energy distribution. While the 9.7 μm feature arises...
We identify a spectroscopic sequence of galaxies, analogous to the Hubble sequence of morphological types, based on the Automatic Spectroscopic K-means-based...
The optical properties of a number of supercompact ultraviolet luminous galaxies (UVLGs), recently discovered in the local universe matching Galaxy Evolution...
Do MURaM and STAGGER Simulations of Solar Faculae Match Observational Signatures from Magnetic Structures?
We compare results of simulations of solar facular-like conditions performed using the numerical codes MURaM and STAGGER. Both simulation sets have a similar...