A SURVEY OF THE LARGE MAGELLANIC CLOUD IN THE [C II] 158 MICRON LINE

被引:57
作者
MOCHIZUKI, K
NAKAGAWA, T
DOI, Y
YUI, YY
OKUDA, H
SHIBAI, H
YUI, M
NISHIMURA, T
LOW, FJ
机构
[1] UNIV TOKYO,FAC SCI,DEPT ASTRON,HONGO 7-1-1,BUNKYO KU,TOKYO 113,JAPAN
[2] UNIV ARIZONA,STEWARD OBSERV,TUCSON,AZ 85724
关键词
GALAXIES; IRREGULAR; ISM; INFRARED; LINES AND BANDS; CLOUDS; MAGELLANIC CLOUDS;
D O I
10.1086/187432
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have mapped the Large Magellanic Cloud (the LMC) in the [C II] 158 mum fine-structure line with the Balloon-borne Infrared Carbon Explorer (BICE) system. The [C II] line emission was detected over most of the LMC. The mean [C II]/CO (J = 1-0) line intensity ratio was 23,000, 18 times larger than the typical value observed in the Galactic plane (1300). This result implies that each clump of the molecular clouds in the LMC has a larger C+ envelope relative to its CO core than those in our Galaxy. Lower dust abundance due to its lower metallicity allows UV photons, which convert CO molecules into C+ ions, to penetrate deeper into the clumps in the LMC than in our Galaxy.
引用
收藏
页码:L37 / L40
页数:4
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