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- W4221010015 abstract "The presence of complex organic molecules (COMs) in the interstellar medium (ISM) is of great interest since it may link to the origin and prevalence of life in the universe. Aiming to investigate the occurrence of COMs and their possible origins, we conducted a chemical census toward a sample of protostellar cores as part of the ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP) project. We report the detection of 11 hot corino sources, which exhibit compact emissions from warm and abundant COMs, among 56 Class 0/I protostellar cores. All the hot corino sources discovered are likely Class 0 and their sizes of the warm region ($>$ 100 K) are comparable to 100 au. The luminosity of the hot corino sources exhibits positive correlations with the total number of methanol and the extent of its emissions. Such correlations are consistent with the thermal desorption picture for the presence of hot corino and suggest that the lower luminosity (Class 0) sources likely have a smaller region with COMs emissions. With the same sample selection method and detection criteria being applied, the detection rates of the warm methanol in the Orion cloud (15/37) and the Perseus cloud (28/50) are statistically similar when the cloud distances and the limited sample size are considered. Observing the same set of COM transitions will bring a more informative comparison between the cloud properties." @default.
- W4221010015 created "2022-04-03" @default.
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- W4221010015 date "2022-03-01" @default.
- W4221010015 modified "2023-10-15" @default.
- W4221010015 title "ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): A Hot Corino Survey toward Protostellar Cores in the Orion Cloud" @default.
- W4221010015 cites W1947770404 @default.
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- W4221010015 cites W2001638972 @default.
- W4221010015 cites W2011759989 @default.
- W4221010015 cites W2012765147 @default.
- W4221010015 cites W2014488392 @default.
- W4221010015 cites W2015400527 @default.
- W4221010015 cites W2016209938 @default.
- W4221010015 cites W2021347355 @default.
- W4221010015 cites W2033172675 @default.
- W4221010015 cites W2033725176 @default.
- W4221010015 cites W2043647577 @default.
- W4221010015 cites W2044669640 @default.
- W4221010015 cites W2046690430 @default.
- W4221010015 cites W2052937506 @default.
- W4221010015 cites W2060647305 @default.
- W4221010015 cites W2075076813 @default.
- W4221010015 cites W2075105883 @default.
- W4221010015 cites W2088673469 @default.
- W4221010015 cites W2091044401 @default.
- W4221010015 cites W2111755119 @default.
- W4221010015 cites W2113951090 @default.
- W4221010015 cites W2117885077 @default.
- W4221010015 cites W2121018712 @default.
- W4221010015 cites W2135625048 @default.
- W4221010015 cites W2140370112 @default.
- W4221010015 cites W2140551581 @default.
- W4221010015 cites W2141099472 @default.
- W4221010015 cites W2143416500 @default.
- W4221010015 cites W2145230401 @default.
- W4221010015 cites W2148804397 @default.
- W4221010015 cites W2157805129 @default.
- W4221010015 cites W2159812255 @default.
- W4221010015 cites W2170292914 @default.
- W4221010015 cites W2193383097 @default.
- W4221010015 cites W2253012927 @default.
- W4221010015 cites W2323604235 @default.
- W4221010015 cites W2640810880 @default.
- W4221010015 cites W2768852965 @default.
- W4221010015 cites W2769898038 @default.
- W4221010015 cites W2770079520 @default.
- W4221010015 cites W2795050267 @default.
- W4221010015 cites W2799056805 @default.
- W4221010015 cites W2799182240 @default.
- W4221010015 cites W2802440906 @default.
- W4221010015 cites W2886067080 @default.
- W4221010015 cites W2888280926 @default.
- W4221010015 cites W2889779774 @default.
- W4221010015 cites W2898332264 @default.
- W4221010015 cites W2904077650 @default.
- W4221010015 cites W2918098937 @default.
- W4221010015 cites W2949316013 @default.
- W4221010015 cites W2964257340 @default.
- W4221010015 cites W2980574950 @default.
- W4221010015 cites W3000663721 @default.
- W4221010015 cites W3003981391 @default.
- W4221010015 cites W3025519223 @default.
- W4221010015 cites W3033111100 @default.
- W4221010015 cites W3036433006 @default.
- W4221010015 cites W3042366190 @default.
- W4221010015 cites W3045115614 @default.
- W4221010015 cites W3092353545 @default.
- W4221010015 cites W3098008896 @default.
- W4221010015 cites W3098382528 @default.
- W4221010015 cites W3098675949 @default.