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NASA NTRS · 20060040740

Dust Coagulation in Infalling Protostellar Envelopes I. Compact Grains

Abstract

Dust plays a key role in the optical, thermodynamic and gas dynamical behavior of collapsing molecular cores. Because of relative velocities of the individual dust grains, coagulation and shattering can modify the grain size distribution and due to corresponding changes in the medium's opacity significantly influence the evolution during early phase of star formation.

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Yorke, H., Suttner, G., Lin, D.. 1999-07-01. Dust Coagulation in Infalling Protostellar Envelopes I. Compact Grains. https://ntrs.nasa.gov/citations/20060040740

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Dust Coagulation in Infalling Protostellar Envelopes I. Compact Grains

Dust plays a key role in the optical, thermodynamic and gas dynamical behavior of collapsing molecular cores. Because of relative velocities of the individual dust grains, coagulation and shattering can modify the grain size distribution and -- due to corresponding changes in the medium's opacity significantly -- influence the evolution during early phases of star formation.

hydrodynamics radiation transfer circumstellar mat↗