Multifluid, magnetohydrodynamic shock waves with grain dynamics. II. Dust and the critical speed for C shocks

Glenn E. Ciolek, Wayne G. Roberge, Telemachos Ch Mouschovias

Research output: Contribution to journalArticle

Abstract

This is the second in a series of papers on the effects of dust on multifluid, magnetohydrodynamic shock waves in weakly ionized molecular gas. We investigate the influence of dust on the critical shock speed, vcrit, above which C shocks cease to exist. Chernoff showed that vcrit cannot exceed the grain magnetosound speed, Vgms, if dust grains are dynamically well coupled to the magnetic field. Since Vgms ≃ 5 km s-1 in a dense cloud or core, the potential implications for models of shock emission are profound. We present numerical simulations of steady shocks where the grains may be well or poorly coupled to the field. We use a time-dependent, multifluid MHD code that models the plasma as a system of interacting fluids: neutral particles, ions, electrons, and various "dust fluids" comprised of grains with different sizes and charges. Our simulations include grain inertia and grain charge fluctuations, but to highlight the essential physics we assume adiabatic flow and single-size grains and neglect the effects of chemistry. We show that the existence of a phase speed vφ does not necessarily mean that C shocks will form for all shock speeds vs less than vφ. When the grains are weakly coupled to the field, steady, adiabatic shocks resemble shocks with no dust: the transition to J-type flow occurs at vcrit ≈ 2.76V nA, where VnA is the neutral Alfvén speed, and steady shocks with vs > 2.76VnA are J shocks with magnetic precursors in the ion-electron fluid. When the grains are strongly coupled to the field, vcrit = min(2.76VnA, V gms). Shocks with vcrit < vs < V gms have magnetic precursors in the ion-electron-dust fluid. Shocks with vs > Vgms have no magnetic precursor in any fluid. We present time-dependent calculations to study the formation of steady, multifluid shocks. The dynamics differ qualitatively, depending on whether or not the grains and field are well coupled.

Original languageEnglish (US)
Pages (from-to)781-800
Number of pages20
JournalAstrophysical Journal
Volume610
Issue number2 I
DOIs
StatePublished - Aug 1 2004

Fingerprint

critical velocity
magnetohydrodynamics
shock wave
shock waves
dust
shock
fluid
electron
ion
inertia
fluids
simulation
physics
grain size
speed
magnetic field
plasma
adiabatic flow
gas
neutral particles

Keywords

  • Dust, extinction
  • ISM: clouds
  • ISM: magnetic fields
  • MHD
  • Plasmas
  • Shock waves

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Multifluid, magnetohydrodynamic shock waves with grain dynamics. II. Dust and the critical speed for C shocks. / Ciolek, Glenn E.; Roberge, Wayne G.; Mouschovias, Telemachos Ch.

In: Astrophysical Journal, Vol. 610, No. 2 I, 01.08.2004, p. 781-800.

Research output: Contribution to journalArticle

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