This book recounts results obtained via the Infrared Space
Observatory (ISO) on comets, in the close environment of pre-main
sequence stars, in the interstellar medium, and in the final stages
of stellar life, using molecular hydrogen, ubiquitous crystalline
silicates, water and ices. ISO has enabled investigation of the
fuelling mechanism of galaxies, and new understanding of luminous
infrared galaxies and their role in shaping present galaxies and in
producing the cosmic infrared background.
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