Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..141h&link_type=abstract
(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),
Astronomy and Astrophysics
Astrophysics
Hydrogen Clouds, Interstellar Magnetic Fields, Magnetic Effects, Magnetohydrodynamic Stability, Nebulae, Shock Waves, Thermal Instability, Density Distribution, Pleiades Cluster, Radiative Heat Transfer
Scientific paper
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.
Hong Seung Sae
Koo Bon-Chul
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