... we may b e witnessing the formation of a molecularcloud out of diffuse atomic gas ... formed indep endently rather than through dislocation from a nearby molecularcloud ...
... of star formation and circumstellar material around young stars), and also with questions of galactic dynamics: the nature of the dark matter in the galactic disc, and the mass and structure of molecularclouds and their interaction with the solar system ...
... The instability of fast shocks in molecularclouds Michael D. Smith and Alexander ... moderately fast shocks in dense molecularclouds with low transverse magnetic fields ...
... may occur near the edges of molecularclouds partially exposed to the ultraviolet ... In molecularclouds that are well shielded from the extreme ultraviolet, the ion ...
... environment on the propagation of protostellar outflows Lindsay Centennial Symposium Outline Introduction Present Study Conclusion Star Formation MolecularClouds 250pc to less than 1pc in extent Masses up to 106 M Densities 10- "Horsehead" nebula 430pc ...
... This may occur edges molecularclouds partially posed to the ultraviolet from nearby ... Unfortunately, molecularclouds, Alfv’en speed uncertain parameter. ... less number, condition expected satisfied molecularclouds (Smith 1993). an analysis ...
... components due to encounters with molecularclouds which exist preferentially in the ... form of nebulae, with cold, dense molecularclouds; although encounters with these ...