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A self-similar solution for thermal disc winds

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journal contribution
posted on 2016-06-08, 15:10 authored by C. Clarke, Richard Alexander
We derive a self-similar description for the 2D streamline topology and flow structure of an axi-symmetric, thermally driven wind originating from a disc in which the density is a power law function of radius. Our scale-free solution is strictly only valid in the absence of gravity or centrifugal support; comparison with 2D hydrodynamic simulations of winds from Keplerian discs however demonstrates that the scale-free solution is a good approximation also in the outer regions of such discs, and can provide a reasonable description even for launch radii well within the gravitational radius of the flow. Although other authors have considered the flow properties along streamlines whose geometry has been specified in advance, this is the first isothermal calculation in which the flow geometry and variation of flow variables along streamlines is determined self-consistently. It is found that the flow trajectory is very sensitive to the power-law index of radial density variation in the disc: the steeper the density gradient, the stronger is the curvature of streamlines close to the flow base that is required in order to maintain momentum balance perpendicular to the flow. Steeper disc density profiles are also associated with more rapid acceleration, and a faster fall-off of density, with height above the disc plane. The derivation of a set of simple governing equations for the flow structure of thermal winds from the outer regions of power law discs offers the possibility of deriving flow observables without having to resort to hydrodynamical simulation.

History

Citation

Monthly Notices of the Royal Astronomical Society, 2016, 460 (3), pp. 3044-3051

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

  • VoR (Version of Record)

Published in

Monthly Notices of the Royal Astronomical Society

Publisher

Oxford University Press (OUP) on behalf of the Royal Astronomical Society

issn

0035-8711

eissn

1365-2966

Acceptance date

2016-05-12

Copyright date

2016

Available date

2016-06-08

Publisher version

http://mnras.oxfordjournals.org/content/460/3/3044

Notes

A correction has been published: Monthly Notices of the Royal Astronomical Society, Volume 482, Issue 2, January 2019, Page 1982, https://doi.org/10.1093/mnras/sty2868 http://hdl.handle.net/2381/45282

Language

en

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