This image from ESO's Very Large Telescope (VLT) shows the newly discovered planet HD95086 b, next to its parent star. The observations were made using NACO, the adaptive optics instrument for the VLT in infrared light, and using a technique called differential imaging, which improves the contrast between the planet and its dazzling host star. The star itself has been removed from the picture during processing to enhance the view of the faint exoplanet and its position is marked. The exoplanet appears at the lower left.

The book covers the whole gamut of optical-IR astronomy from the Solar System, search for planets in nearby stars, physics of Galactic stars and clusters, Galactic structure, structure of nearby galaxies, AGN and quasars, clusters of galaxies, to large structure and cosmology. Furthermore it summarizes the two panel discussions. Many important observational clues about our understanding of how stars and planets form in the interior of molecular clouds have been amassed using recent technological developments. ESO's very large telescope promises to be a major step forward in the investigation of stellar nurseries and infant. T Tauri Stars in the Large Magellanic Cloud: A Combined HST and VLT Effort Martino Romaniello, Nino Panagia, Salvatore Scuderi, Roberto Gilmozzi, Eline Tolstoy, Fabio Favata et al.

The blue circle is the size of the orbit of Neptune in the Solar System.

The star HD 95086 has similar properties to Beta Pictoris and HR 8799 around which giant planets have previously been imaged at separations between 8 and 68 astronomical units. These stars are all young, more massive than the Sun, and surrounded by a debris disc.

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