|
|
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. |
|
|
|
|