Clustering and dynamic decoupling of dust grains in turbulent molecular clouds

Research output: Contribution to journalArticleScientificpeer-review

Researchers

Research units

  • NORDITA
  • Uppsala University

Abstract

We present high-resolution (1024 3) simulations of super-/hypersonic isothermal hydrodynamic turbulence inside an interstellar molecular cloud (resolving scales of typically 20-100 au), including a multidisperse population of dust grains, i.e. a range of grain sizes is considered. Due to inertia, large grains (typical radius a ≳ 1.0μm) will decouple from the gas flow, while small grains (al∼ 0.1μm) will tend to better trace the motions of the gas. We note that simulations with purely solenoidal forcing show somewhat more pronounced decoupling and less clustering compared to simulations with purely compressive forcing. Overall, small and large grains tend to cluster, while intermediate-size grains show essentially a random isotropic distribution. As a consequence of increased clustering, the grain-grain interaction rate is locally elevated; but since small and large grains are often not spatially correlated, it is unclear what effect this clustering would have on the coagulation rate. Due to spatial separation of dust and gas, a diffuse upper limit to the grain sizes obtained by condensational growth is also expected, since large (decoupled) grains are not necessarily located where the growth species in the molecular gas is.

Details

Original languageEnglish
Pages (from-to)5623–5641
Number of pages19
JournalMonthly Notices of the Royal Astronomical Society
Volume483
Issue number4
Publication statusPublished - 11 Mar 2019
MoE publication typeA1 Journal article-refereed

    Research areas

  • dust, extinction, hydrodynamics, instabilities

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