Abstract
The effect of a magnetic field on a thermal instability has been studied in a radiatively cooling region behind an interstellar shock of moderate propagation velocity (∼ 10 km s−1). It is shown that the presence of a magnetic field of a few microgauss is very effective in preventing the thermal instability from building-up density concentrations. In the absence of the magnetic field, the shock-induced thermal instability will amplify a pre-shock density inhomogeneity by more than an order of magnitude. However, in the field's presence, the amplified density contrast is shown to be only a factor 2. Implications for the ‘trace of a sweeping broom’ in the Pleiades nebula are discussed.
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Hong, S.S., Koo, B.C. Effect of magnetic field on a shock-induced thermal instability. Astrophys Space Sci 119, 141–142 (1986). https://doi.org/10.1007/BF00648832
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DOI: https://doi.org/10.1007/BF00648832