Dust coagulation during the early stages of star formation: molecular cloud collapse and first hydrostatic core evolution
Matthew R. Bate
Abstract
This is the author accepted manuscript. The final version is available on open access from Oxford University Press via the DOI in this record
Topics & Concepts
PhysicsAstrophysicsMolecular cloudHydrostatic equilibriumStar formationInterstellar mediumGrain growthCore (optical fiber)Dust laneYoung stellar objectAstronomyGrain sizeStarsGalaxyOpticsMaterials scienceMetallurgyAstrophysics and Star Formation StudiesMolecular Spectroscopy and StructureAdvanced Combustion Engine Technologies