Smith, M.D. (1992) Switch shocks in molecular clouds. I. Plane-parallel magnetohydrodynamic analysis. Astrophysical Journal, 390 (2). pp. 447-453. ISSN 0004-637X. (doi:10.1086/171295) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:50163)
The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided. | |
Official URL: http://dx.doi.org/10.1086/171295 |
Abstract
Magnetohydrodynamic shock waves in molecular clouds are discussed. Plane-parallel flows with oblique magnetic fields are analyzed with particular regard to switch shocks. Switch-on shocks occur in the limit as the flow and field directions coincide; a transverse field is then switched on by the shock. In molecular clouds these become continuous or C-type, here termed C-switches. Their existence rules out the alternative J-type hydrodynamic flows. J-switches are only possible at low Alfvén numbers even in strongly radiative shocks which possess an equilibrium temperature. C-switches yield both strong compression and large swings in the magnetic field direction. They arise under a wide range of general conditions. One requirement is that the Alfvén speed exceeds the sound speed. The other requirement, to keep the flow supersonic, is that A2/?0 is small, where A is the Alfvén number and ?0 is a ratio of heating to cooling time scales. For transverse-field shocks the weaker restraint is on A/?0. Upstream and downstream flow behavior is examined; weak downstream subshocks are more probable in C-switches than in transverse shocks. The temperature profile across an oblique shock is derived using the cool C-shock method. A formula is presented which determines the transverse shock of equivalent excitation. C-switch behavior influences flows within an angle ?1/A of the field direction. Switch-off C-shocks, in which the field pressure generated by the switch-on shock is converted into thermal pressure as the transverse field disappears, are also discussed. An approximate isothermal solution is found.
Item Type: | Article |
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DOI/Identification number: | 10.1086/171295 |
Uncontrolled keywords: | ISM: molecules, MHD shock waves |
Subjects: | Q Science > QB Astronomy > QB460 Astrophysics |
Divisions: | Divisions > Division of Natural Sciences > Physics and Astronomy |
Depositing User: | Giles Tarver |
Date Deposited: | 11 Aug 2015 10:42 UTC |
Last Modified: | 05 Nov 2024 10:35 UTC |
Resource URI: | https://kar.kent.ac.uk/id/eprint/50163 (The current URI for this page, for reference purposes) |
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