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Carbon-chain molecules in molecular outflows and Lupus I region – New producing region and new forming mechanism
dc.contributor.author | Wu Y. | |
dc.contributor.author | Liu X. | |
dc.contributor.author | Chen X. | |
dc.contributor.author | Lin L. | |
dc.contributor.author | Yuan J. | |
dc.contributor.author | Zhang C. | |
dc.contributor.author | Liu T. | |
dc.contributor.author | Shen Z. | |
dc.contributor.author | Li J. | |
dc.contributor.author | Wang J. | |
dc.contributor.author | Qin S.-L. | |
dc.contributor.author | Kim K.-T. | |
dc.contributor.author | Liu H. | |
dc.contributor.author | Zhu L. | |
dc.contributor.author | Madones D. | |
dc.contributor.author | Inostroza N. | |
dc.contributor.author | Henkel C. | |
dc.contributor.author | Zhang T. | |
dc.contributor.author | Li D. | |
dc.contributor.author | Esimbek J. | |
dc.contributor.author | Liu Q. | |
dc.date.accessioned | 2020-09-02T22:30:34Z | |
dc.date.available | 2020-09-02T22:30:34Z | |
dc.date.issued | 2019 | |
dc.identifier | 10.1093/mnras/stz1498 | |
dc.identifier.issn | 00358711 | |
dc.identifier.uri | https://hdl.handle.net/20.500.12728/6635 | |
dc.description | Using the new equipment of the Shanghai Tian Ma Radio Telescope, we have searched for carbon-chain molecules (CCMs) towards five outflow sources and six Lupus I starless dust cores, including one region known to be characterized by warm carbon-chain chemistry (WCCC), Lupus I-1 (IRAS 15398-3359), and one TMC-1 like cloud, Lupus I-6 (Lupus-1A). Lines of HC3N J = 2 − 1, HC5N J = 6 − 5, HC7N J = 14 − 13, 15 − 14, 16 − 15, and C3S J = 3 − 2 were detected in all the targets except in the outflow source L1660 and the starless dust core Lupus I-3/4. The column densities of nitrogen-bearing species range from 1012 to 1014 cm−2 and those of C3S are about 1012 cm−2. Two outflow sources, I20582+7724 and L1221, could be identified as new carbon-chain-producing regions. Four of the Lupus I dust cores are newly identified as early quiescent and dark carbon-chain-producing regions similar to Lup I-6, which together with the WCCC source, Lup I-1, indicate that carbon-chain-producing regions are popular in Lupus I which can be regard as a Taurus-like molecular cloud complex in our Galaxy. The column densities of C3S are larger than those of HC7N in the three outflow sources I20582, L1221, and L1251A. Shocked carbon-chain chemistry is proposed to explain the abnormal high abundances of C3S compared with those of nitrogen-bearing CCMs. Gas-grain chemical models support the idea that shocks can fuel the environment of those sources with enough S+ thus driving the generation of S-bearing CCMs. © 2019 The Author(s). | |
dc.language.iso | en | |
dc.publisher | Oxford University Press | |
dc.subject | ISM: abundance | |
dc.subject | ISM: jets and outflows | |
dc.subject | ISM: kinematics and dynamics | |
dc.subject | ISM: molecules | |
dc.subject | Stars: formation | |
dc.title | Carbon-chain molecules in molecular outflows and Lupus I region – New producing region and new forming mechanism | |
dc.type | Article |