Dust Growth in Molecular Cloud Envelopes: A Numerical Approach

Variations in the grain size distribution are to be expected in the interstellar medium (ISM) owing to grain growth and destruction. In this work, we present a dust collision model to be implemented inside a magnetohydrodynamic (MHD) code that takes into account grain growth and shattering of charge...

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Veröffentlicht in:	The Astrophysical journal 2021-03, Vol.909 (2), p.206
Hauptverfasser:	Beitia-Antero, Leire, Gómez de Castro, Ana I.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Building codes Charged particles Coagulation Computational fluid dynamics Dust Equations of motion Extinction Filaments Fluid flow Grain growth Grain size Grain size distribution Graphite Interstellar matter Interstellar medium Magnetohydrodynamics Molecular clouds Particle size Particle size distribution Silicates
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