ORION-B (NGC-2024) .3. BIMA SO JK=2(2)-]1(1) OBSERVATIONS - EVIDENCE FOR PECULIAR SULFUR CHEMISTRY

被引:3
作者
BARNES, PJ
CRUTCHER, RM
机构
[1] UNIV TORONTO,CANADIAN INST THEORET ASTROPHYS,MCLENNAN PHYS LABS,TORONTO M5S 1A1,ONTARIO,CANADA
[2] UNIV ILLINOIS,DEPT ASTRON,URBANA,IL 61801
关键词
ISM INDIVIDUAL (NGC-2024); ISM MOLECULES; ISM STRUCTURE; MOLECULAR PROCESSES;
D O I
10.1086/171207
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present aperture synthesis maps of SO J(K) = 2(2) --> 1(1) emission at 86.093938 GHZ of the molecular cloud Orion B obtained from combined BIMA/NRAO 12 m data. The spatial resolution is 11" x 7" and the velocity resolution is 0.54 km s-1. The maps show fine structure in the dense molecular core, the main features being two relatively compact components aligned with the long, quiescent, NS-oriented ridge of previous maps. Most notable, however, is the approximately 1-2 km s-1 blueshift of this line with respect to other high-density tracers of the main core. implications of these data for the chemistry of SO in dense clouds are discussed.
引用
收藏
页码:325 / 337
页数:13
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