Ambipolar diffusion, interstellar dust, and the formation of cloud cores and protostars. I. Basic physics and formulation of the problem

Glenn E. Ciolek, Telemachos Ch Mouschovias

Research output: Contribution to journalArticle

Abstract

We formulate the problem of the self-initiated formation and contraction of cloud cores due to ambipolar diffusion in axisymmetric, self-gravitating, isothermal, magnetic molecular cloud models, accounting for a cosmic abundance of interstellar grains (both charged and neutral). The basic microscopic and macroscopic effects of grains are discussed. The magnetohydrodynamic equations for a multicomponent plasma are derived, the dimensionless free parameters are obtained, and their meaning is explained physically. The ion and electron fluids combine to form a system of "quasiparticles," each having an effective charge Zeff = e(ni - ne)/ni (where ni and ne are the number densities of ions and electrons, and e the electronic charge). Electrostatic attraction between quasiparticles, which are attached to the magnetic field, and negatively charged grains couples the grains to the field even at densities at which grain-neutral collisions would normally decouple the grains from the field. Also, neutral grains can couple to the magnetic field through (inelastic) charge capture. The numerical method of solution, the results, and their application to the formation of cores and protostars in molecular clouds are presented in following papers.

Original languageEnglish (US)
Pages (from-to)774-793
Number of pages20
JournalAstrophysical Journal
Volume418
Issue number2
DOIs
StatePublished - Dec 1 1993

Fingerprint

ambipolar diffusion
protostars
physics
dust
magnetic field
formulations
electron
ion
magnetohydrodynamics
numerical method
contraction
collision
plasma
fluid
molecular clouds
magnetic fields
attraction
ions
electrons
electrostatics

Keywords

  • Diffusion
  • Dust: extinction
  • ISM: magnetic fields
  • MHD
  • Plasmas
  • Stars: formation

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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abstract = "We formulate the problem of the self-initiated formation and contraction of cloud cores due to ambipolar diffusion in axisymmetric, self-gravitating, isothermal, magnetic molecular cloud models, accounting for a cosmic abundance of interstellar grains (both charged and neutral). The basic microscopic and macroscopic effects of grains are discussed. The magnetohydrodynamic equations for a multicomponent plasma are derived, the dimensionless free parameters are obtained, and their meaning is explained physically. The ion and electron fluids combine to form a system of {"}quasiparticles,{"} each having an effective charge Zeff = e(ni - ne)/ni (where ni and ne are the number densities of ions and electrons, and e the electronic charge). Electrostatic attraction between quasiparticles, which are attached to the magnetic field, and negatively charged grains couples the grains to the field even at densities at which grain-neutral collisions would normally decouple the grains from the field. Also, neutral grains can couple to the magnetic field through (inelastic) charge capture. The numerical method of solution, the results, and their application to the formation of cores and protostars in molecular clouds are presented in following papers.",
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N2 - We formulate the problem of the self-initiated formation and contraction of cloud cores due to ambipolar diffusion in axisymmetric, self-gravitating, isothermal, magnetic molecular cloud models, accounting for a cosmic abundance of interstellar grains (both charged and neutral). The basic microscopic and macroscopic effects of grains are discussed. The magnetohydrodynamic equations for a multicomponent plasma are derived, the dimensionless free parameters are obtained, and their meaning is explained physically. The ion and electron fluids combine to form a system of "quasiparticles," each having an effective charge Zeff = e(ni - ne)/ni (where ni and ne are the number densities of ions and electrons, and e the electronic charge). Electrostatic attraction between quasiparticles, which are attached to the magnetic field, and negatively charged grains couples the grains to the field even at densities at which grain-neutral collisions would normally decouple the grains from the field. Also, neutral grains can couple to the magnetic field through (inelastic) charge capture. The numerical method of solution, the results, and their application to the formation of cores and protostars in molecular clouds are presented in following papers.

AB - We formulate the problem of the self-initiated formation and contraction of cloud cores due to ambipolar diffusion in axisymmetric, self-gravitating, isothermal, magnetic molecular cloud models, accounting for a cosmic abundance of interstellar grains (both charged and neutral). The basic microscopic and macroscopic effects of grains are discussed. The magnetohydrodynamic equations for a multicomponent plasma are derived, the dimensionless free parameters are obtained, and their meaning is explained physically. The ion and electron fluids combine to form a system of "quasiparticles," each having an effective charge Zeff = e(ni - ne)/ni (where ni and ne are the number densities of ions and electrons, and e the electronic charge). Electrostatic attraction between quasiparticles, which are attached to the magnetic field, and negatively charged grains couples the grains to the field even at densities at which grain-neutral collisions would normally decouple the grains from the field. Also, neutral grains can couple to the magnetic field through (inelastic) charge capture. The numerical method of solution, the results, and their application to the formation of cores and protostars in molecular clouds are presented in following papers.

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