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- W4380032743 abstract "Abstract The depletion of CO molecules is observed in infrared dark clouds. However, only few exsamples are found in pc-scale. An NH 3 emission is one of good counter parts of C 18 O because of similar effective critical density. Our NH 3 observations of a molecular filament associated with CMa OB1 or KAG 71, which is a target of Kagoshima Galactic Object survey with Nobeyama 45-m telescope by Mapping in Ammonia lines (KAGONMA) project. Although NH 3 data shows similarity in morphology with infrared data suggesting no depletion, C 18 O in the clumps 4 and 6 are weaker than expected based on NH 3 data. After examining the dissipation of the high-density gas, photodissociation, and depletion, we concluded that CO is depleted at least in the clump 4. It is a new example of depletion in pc-scale." @default.
- W4380032743 created "2023-06-10" @default.
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- W4380032743 date "2021-08-01" @default.
- W4380032743 modified "2023-10-07" @default.
- W4380032743 title "Parsec scale CO depletion in KAGONMA 71, or a star-forming filament in CMa OB1" @default.
- W4380032743 doi "https://doi.org/10.1017/s1743921322004926" @default.
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