The chemical signature of magnetohydrodynamic waves in molecular clouds

被引:10
作者
Charnley, SB
机构
[1] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[2] NASA, Div Space Sci, Ames Res Ctr, Moffett Field, CA 94035 USA
关键词
MHD; molecular processes; ISM : clouds; ISM : molecules;
D O I
10.1046/j.1365-8711.1998.01757.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
By considering the propagation of low-amplitude magnetohydrodynamic waves in partially ionized plasmas, it is shown that the ion-neutral drift (ambipolar diffusion) induced by the waves can have specific effects on the molecular chemistry of cold material. The chemistry occurring in gas swept by Alfven waves is described and it is shown that this leads to spatial variations in the deuterium fractionation ratios of, for example, HCO+ and N2H+, on spatial scales of a few hundredths of a parsec, depending upon the fractional ionization of the ambient medium. The possibility of detecting interstellar Alfven waves by molecular spectroscopy and their effect of producing small-scale chemical abundance gradients in molecular clouds are briefly discussed.
引用
收藏
页码:L25 / L28
页数:4
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