SURPRISINGLY HIGH-PRESSURE SHOCKS IN THE SUPERNOVA REMNANT IC-443

被引:19
作者
MOORHOUSE, A
BRAND, PWJL
GEBALLE, TR
BURTON, MG
机构
[1] ROYAL OBSERV,DEPT ASTRON,EDINBURGH EH9 3HJ,MIDLOTHIAN,SCOTLAND
[2] JOINT ASTRON CTR,HILO,HI 96720
[3] NASA,AMES RES CTR,MOFFETT FIELD,CA 94035
[4] UNIV CALIF IRVINE,IRVINE,CA 92717
基金
美国国家航空航天局;
关键词
D O I
10.1093/mnras/253.4.662
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The intensities of several lines of molecular hydrogen have been measured from two regions of the supernova-remnant/molecular-cloud shock in IC443. The lines measured have upper-state energies ranging from 7000 K to 23 000 K. Their relative intensities differ in the two regions, but are consistent with those predicted from the post-shock regions of simple jump-type shocks of different pressure. The pressures so derived are far higher than the pressure in the supernova remnant itself, and a possible reason for this discrepancy is discussed.
引用
收藏
页码:662 / 668
页数:7
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