Titlebook: Astronomie spatiale infrarouge, aujourd‘hui et demain Infrared space astronomy, today and tomorrow; 3-28 August 1998 F. Casoli,J. Lequeux,F

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Cosmology with ISO,n with the so—called semi—analytic approach of galaxy formation are outlined. A preview of survey capabilities with forthcoming instruments after ISO shows that our knowledge of the “optically—dark” side of the universe should increase rapidly.

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0924-8099 quality lectures should attract a wide audience..Includes suThis book brings together the lectures given at the Les Houches summer school "Infrared space astronomy, today and tomorrow". It gives a wide overview of infrared astronomy, a wavelength domain crucial for studies of the solar system, stars

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Fortschritte der Hochpolymeren-Forschungre and how stars make atoms heavier than helium: such questions have occupied the minds of astrophysicists in the first 2/3 of this century and the satisfactory answers to all this questions is undoubtedly one of the major successes of astrophysics in this century.

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Stars and Galactic Structure,re and how stars make atoms heavier than helium: such questions have occupied the minds of astrophysicists in the first 2/3 of this century and the satisfactory answers to all this questions is undoubtedly one of the major successes of astrophysics in this century.

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Conference proceedings 2000 of infrared astronomy, a wavelength domain crucial for studies of the solar system, stars at the beginning and end of their lives, interstellar matter and galaxies at all distances. Recent developments in observational techniques have been tremendous. The first contributions give an introduction to

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Overview of the ISO Mission,n-orbit performance of the satellite and its four scientific instruments, the operational scenario and some of the scientific highlights. It then focusses on ISO’s legacy to the astronomical community, giving an overview of the ISO data archive, its contents, access methods, available software tools and overall documentation.

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L. E. Coleman Jr.,N. A. Meinhardtibuted to our knowledge of the processes in question, with particular emphasis on the ISO contributions. This order, . from theory to observations, has been chosen mostly for heuristic purposes. In reality, often observations have preceded and motivated theories, rather than vice-versa.