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Early-stage star-forming cloud cores in Galactic Legacy Infrared Mid-Plane Survey (GLIMPSE) extended green objects (EGOs) as traced by organic species
Ge, J. X.1,2; He, J. H.1; Chen, X.3,4; Takahashi, S.5,6,7
2014-12-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume445Issue:2Pages:1170-1185
AbstractIn order to investigate the physical and chemical properties of massive star-forming cores in the early stages, we analyse the excitation and abundance of four organic species, CH3OH, CH3OCH3, HCOOCH3 and CH3CH2CN, towards 29 extended green object (EGO) cloud cores that were observed by our previous single-dish spectral line survey. The EGO cloud cores are found to have similar methanol J(3)-J(2) rotation temperatures of similar to 44 K, a typical linear size of similar to 0.036 pc and a typical beam-averaged methanol abundance of several 10(-9) (the beam-corrected value could reach several 10(-7)). The abundances of the latter three species, normalized by that of methanol, are also found to be correlated across a large variety of clouds such as EGO cloud cores, hot corinos, massive hot cores and Galactic Centre clouds. The chemical properties of the EGO cloud cores lie between those of hot cores and hot corinos. However, the abundances and abundance ratios of the four species cannot be explained satisfactorily by recent chemical models, either among EGO cloud cores or among the various types of cloud core from literature.
KeywordAstrochemistry Ism: Abundances Ism: Clouds Ism: Evolution Ism: Molecules Submillimetre: Ism
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1093/mnras/stu1758
WOS KeywordMOLECULAR CLOUDS ; DARK CLOUDS ; HOT-CORE ; CLASS-I ; MASSIVE STARS ; INITIAL CONDITIONS ; COLOGNE DATABASE ; METHANOL MASERS ; HIGH-RESOLUTION ; SAGITTARIUS B2
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000346959400008
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Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/15735
Collection暗物质和空间天文实验室
Affiliation1.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Yunnan Observ, Kunming 650011, Yunnan Province, Peoples R China
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China
4.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China
5.Joint ALMA Observ, Santiago, Chile
6.Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan
7.Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan
Recommended Citation
GB/T 7714
Ge, J. X.,He, J. H.,Chen, X.,et al. Early-stage star-forming cloud cores in Galactic Legacy Infrared Mid-Plane Survey (GLIMPSE) extended green objects (EGOs) as traced by organic species[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2014,445(2):1170-1185.
APA Ge, J. X.,He, J. H.,Chen, X.,&Takahashi, S..(2014).Early-stage star-forming cloud cores in Galactic Legacy Infrared Mid-Plane Survey (GLIMPSE) extended green objects (EGOs) as traced by organic species.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,445(2),1170-1185.
MLA Ge, J. X.,et al."Early-stage star-forming cloud cores in Galactic Legacy Infrared Mid-Plane Survey (GLIMPSE) extended green objects (EGOs) as traced by organic species".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 445.2(2014):1170-1185.
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