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Gravitational instability of partially ionized molecular clouds

Published online by Cambridge University Press:  01 December 2007

A.C. BORAH and
A.K. SEN
A.C. BORAH
Affiliation:
Department of Physics, Assam University, Silchar 788011, India
A.K. SEN
Affiliation:
Department of Physics, Assam University, Silchar 788011, India
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Abstract

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Stars are formed as a result of the gravitational (Jeans) collapse of dense clumps in interstellar clouds. These clouds are partially ionized by nearby ionizing sources. We investigate the gravitational instability in such molecular clouds considering the non-Boltzmannian distribution for electrons and ions, which is more realistic than the Boltzmannian distribution. Assuming the perturbation (fluctuation) response in a radial direction as a mathematical analogue of the x-direction in the plane geometry approximation in the form f ∼ exp(ikx–iωt), the equations of motion for different species of the multi-fluid plasma are linearized. Jeans' swindle is used as a local approximation for the equilibrium and the dispersion relation is derived by usual normal mode analysis. Then, an analytical solution to the dispersion equation with an explanation of the effects on star formation is given.

Information

Type
Papers
Information
Journal of Plasma Physics , Volume 73 , Issue 6 , December 2007, pp. 831 - 838
Copyright
Copyright © Cambridge University Press 2007

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