Shock Chemistry in Low-Mass Star-Forming Regions

被引:0
|
作者
Yamaguchi, Takahiro [1 ]
Takano, Shuro [2 ,3 ]
Sakai, Nami [1 ]
Watanabe, Yoshimasa [1 ]
Yamamoto, Satoshi [1 ]
机构
[1] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan
[2] Grad Univ Adv Studies Sokendai, Nobeyama Radio Observ, Minamisa Ku, Minamimaki, Nagano 3841305, Japan
[3] Grad Univ Adv Studies Sokendai, Dept Astron Sci, Minamisa Ku, Minamimaki, Nagano 3841305, Japan
关键词
SPECTRAL-LINE SURVEY; PHOSPHORUS;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have conducted spectral line surveys in the 3 mm band with the 45 m telescope of the Nobeyama Radio Observatory toward the L1157 B1 and L1448 B1/R1 shocked regions. L1157 B1 is a famous shocked region formed by the interaction between the outflow from the protostar IRAS 20386+6751 and the ambient gas, while L1448 B1/R1 are formed from internal bow shocks within the extremely energetic jet from the protostar L1448 mm. As a result, we found a grate difference of the chemical composition between the two shocked regions.
引用
收藏
页码:321 / 322
页数:2
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