Titlebook: Chemistry in Space; J. M. Greenberg,V. Pirronello Book 1991 Kluwer Academic Publishers 1991 LOPES.Supernova.collision.cosmic ray.interstel

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Molecular Clouds in Regions of Massive Star Formationar neighborhood (G0≈ 1.6×10. erg s. cm.). Furthermore, massive stars also have supersonic winds with velocities up to several thousand km/s carrying between 0.1 and 1% of the star’s luminosity in form of kinetic energy. At the end of its lifetime an 0 star explodes as a supernova, ejecting 10. erg o

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