Titlebook: Science with the VLT Interferometer; Proceedings of the E Francesco Paresce Conference proceedings 1997 Springer-Verlag Berlin Heidelberg 1

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Direct Observation of Extrasolar Planets with an Infrared Interferometery 10. – 10. in the best cases), but not impossible if a very careful spatial filtering and calibration is imposed upon the recombined beams..We propose an observing strategy to monitor hot extrasolar planets of the 51 Peg class, for which the VLTI provides sufficient sensitivity and adequate baselines.

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VLTI Observations of Radio-Loud Active GalaxiesI shall consider the relevance of VLTI for studying the nuclear regions of radio-loud galaxies and quasars. Various scientific drivers for observing these objects will be discussed and the feasibility of such observations will be appraised, given the expected angular resolutions and sensitivities.

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ugh different marketing methods, to find customers. It becomes obvious, therefore, for the companies that manufacturing a product is much easier than marketing it nowadays. After taking into consideration, the costs for all stages of development, production and marketing, it is rather hard to find a

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Timothy R. Beddinglting from fuel combustion. As documented earlier in the literature, the energy consumption has one of the most important influences on the carbon emissions. Nevertheless, there is no agreement about the role of renewables in environmental protection. Further, the endogeneity effect between CO. emis

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