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Paper: Shock Chemistry in Low-Mass Star-Forming Regions
Volume: 476, New Trends in Radio Astronomy in the ALMA Era
Page: 321
Authors: Yamaguchi, T.; Takano, S.; Sakai, N.; Watanabe, Y.; Yamamoto, S.; NRO Line Survey Team Members
Abstract: 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.
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