THE H-2 LINE-PROFILES IN THE CYGNUS LOOP - EVIDENCE FOR J-SHOCKS WITH MAGNETIC PRECURSORS

被引:8
作者
GRAHAM, JR [1 ]
WRIGHT, GS [1 ]
GEBALLE, TR [1 ]
机构
[1] JOINT ASTRON CTR,HILO,HI 96720
关键词
D O I
10.1086/186014
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have obtained infrared Fabry-Perot spectra at almost-equal-to 25 km s-1 resolution of the H-2 line emission associated with the fast shocks to the NE of the Cygnus Loop supernova remnant. Profiles of the 1-0 S(1) H-2 emission associated with both the optically bright radiative shocks and the faint nonradiative shocks have been observed. The profiles are resolved and have deconvolved widths of almost-equal-to 20 km s-1. This result favors excitation of the H-2 emission in a magnetic precursor over excitation by a radiative precursor. Shocks with precursors may play an important role in Herbig-Haro objects, and in star-forming cloud cores.
引用
收藏
页码:L21 / L24
页数:4
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