MOLECULAR SIGNATURES OF MHD WAVES

被引：6

作者：

CHARNLEY, SB

BUTNER, H

机构：

[1] NASA, AMES RES CTR, DIV SPACE SCI, MOFFETT FIELD, CA 94035 USA

[2] CARNEGIE INST WASHINGTON, DEPT TERR MAGNETISM, WASHINGTON, DC 20005 USA

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1995年 / 224卷 / 1-2期

关键词：

ISM; MOLECULES; KINEMATICS AND DYNAMICS;

D O I：

10.1007/BF00667896

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The small ion-neutral drift speeds attained in MHD waves lead to a significant increase in the rates of several important ion-molecule reactions. The effect on the deuterium chemistry of dark clouds could allow MHD wave motion to be observed directly. The results of some recent observations to test this theory are outlined.

引用

页码：443 / 444

页数：2

共 7 条

[1] BUTNER H, 1994, UNPUB
[2] CHARNLEY SB, 1992, IAU SYMP, V150, P155
[3] CHARNLEY SB, 1994, UNPUB
[4] DEUTERIUM FRACTIONATION IN DENSE INTERSTELLAR CLOUDS
MILLAR, TJ
BENNETT, A
HERBST, E
[J]. ASTROPHYSICAL JOURNAL, 1989, 340 (02) : 906 - 920
[5] OLANO CA, 1988, ASTRON ASTROPHYS, V196, P194
[6] A SOURCE MODEL FOR THE L134N MOLECULAR CLOUD
SWADE, DA
SCHLOERB, FP
[J]. ASTROPHYSICAL JOURNAL, 1992, 392 (02) : 543 - 550
[7] HYDROMAGNETIC WAVE DISSIPATION IN MOLECULAR CLOUDS
ZWEIBEL, EG
JOSAFATSSON, K
[J]. ASTROPHYSICAL JOURNAL, 1983, 270 (02) : 511 - 518

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