Millimeter observations of organic molecules toward high-mass star   formation region G34.26+0.15

doi:10.1088/1674-4527/16/12/182

CORC > 北京大学 > 化学与分子工程学院

	Millimeter observations of organic molecules toward high-mass star formation region G34.26+0.15
	Fu, Li ; Lin, Guo-Man
刊名	RESEARCH IN ASTRONOMY AND ASTROPHYSICS
	2016
关键词	astrochemistry molecular processes line: identification ISM: abundances GRAIN-SURFACE-CHEMISTRY H-II-REGIONS HIGH-RESOLUTION HII-REGIONS LINE EMISSION COMPLEX CORE ABUNDANCES
DOI	10.1088/1674-4527/16/12/182
英文摘要	To investigate the chemical origination of organic molecules CH3OH, CH3OCH3, C2H5OH, CH3OCH, CH3CN, C2H3CN and C2H5CN in the hot core associated with high-mass star formation region G34.26+0.15, Submillimeter Array observations were made with its 230 GHz receiver. The molecular gas distribution has shown that the oxygen- and nitrogen-containing molecules peak at different positions. Comparing the spatial distributions with rotational temperatures and fractional abundances of the observed molecules, we discuss the possible chemical origination of these organic molecules.; Specialized Research Fund for the Program of Langfang Teachers University, China [LSLZ 201401]; Natural Science Foundation of Hebei Province, China [B2014408013]; SCI(E); 中国科技核心期刊(ISTIC); ARTICLE; fuli668@126.com; 12; 16
语种	英语
内容类型	期刊论文
源URL	[http://ir.pku.edu.cn/handle/20.500.11897/458193]
专题	化学与分子工程学院
推荐引用方式 GB/T 7714	Fu, Li,Lin, Guo-Man. Millimeter observations of organic molecules toward high-mass star formation region G34.26+0.15[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2016.
APA	Fu, Li,&Lin, Guo-Man.(2016).Millimeter observations of organic molecules toward high-mass star formation region G34.26+0.15.RESEARCH IN ASTRONOMY AND ASTROPHYSICS.
MLA	Fu, Li,et al."Millimeter observations of organic molecules toward high-mass star formation region G34.26+0.15".RESEARCH IN ASTRONOMY AND ASTROPHYSICS (2016).