The metallicity distribution of stars in the Fornax dwarf spheroidal galaxy is studied with infrared Ca II triplet spectroscopy for 117 red giants, obtained with FORS1 on the VLT. The results reveal a very wide distribution of metallicities in Fornax, including a surprising abundance of young, relatively metal-rich stars ([Fe/H]>-0.7). By combining

. Superstatistics is a superposition of two different statistics relevant to driven nonequilibrium systems with a stationary state and intensive parameter fluctuations. It contains Tsallis statistics as a special case. After briefly summarizing some of the theoretical aspects, we describe recent applications of this concept to three different

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We summarize in this paper the principles for the algorithmic representation of the structure of a stellar atmosphere. The physical analysis of the problem leads to the classification of the elementary blocks that constitute a stellar atmosphere model and suggest the numerical algorithms required for its computation. Compatibly with the space

Using the NOT, WHT and TNG telescopes located at Observatorio del Roque de los Muchachos (Canary Islands, Spain) we have obtained low resolution visible and near infrared spectra of more than 30 Near Earth Asteroids. These observations are part of and observational campaign that started on August 2002 and that also includes photometric and

Gravity modes are the best probes to study the solar radiative zone, in particular the nuclear core and to follow its potential variability with time and latitude. Nevertheless, their amplitude is small and the solar noise particularly high in the range of frequency where they stand (below 500 μ Hz). It is why they are looked for more than 20 years