H2CO and H110 alpha Observations toward the Aquila Molecular Cloud

doi:10.3847/1538-4357/ab0ae3

	H2CO and H110 alpha Observations toward the Aquila Molecular Cloud
	Komesh, Toktarkhan 1,2,3; Esimbek, Jarken 1,4; Baan, Willem 1,5; Zhou, Jianjun 1,4; Li, Dalei 1,4; Wu, Gang 1,4; He, Yuxin 1,4; Sailanbek, Serikbek 1,2,3; Tang, Xindi 1,4; Manapbayeva, Arailym 1,2
刊名	ASTROPHYSICAL JOURNAL
	2019-04-01
卷号	874 期号:2 页码:10
关键词	ISM: molecules stars: formation
ISSN号	0004-637X
DOI	10.3847/1538-4357/ab0ae3
通讯作者	Komesh, Toktarkhan(toktarhan@xao.ac.cn)
英文摘要	The formaldehyde H2CO(1(10) -1(11) ) absorption line and H110 alpha radio recombination line have been observed toward the Aquila Molecular Cloud using the Nanshan 25 m telescope operated by the Xinjiang Astronomical Observatory CAS. These first observations of the H2CO (1(10) -1(11) ) absorption line determine the extent of the molecular regions that are affected by the ongoing star formation in the Aquila molecular complex and show some of the dynamic properties. The distribution of the excitation temperature T-ex for H2CO identifies the two known star formation regions W40 and Serpens South as well as a smaller new region Serpens 3. The intensity and velocity distributions of H2CO and (CO)-C-13(1-0) do not agree well with each other, which confirms that the H2CO absorption structure is mostly determined by the excitation of the molecules resulting from the star formation rather than by the availability of molecular material as represented by the distribution. Some velocity-coherent linear (CO)-C-13(1-0) structures have been identified in velocity channel maps of H2CO and it is found that the three star formation regions lie on the intersect points of filaments. The H110 alpha emission is found only at the location of the W40 H II region and spectral profile indicates a redshifted spherical outflow structure in the outskirts of the H II region. Sensitive mapping of H2CO absorption of the Aquila Complex has correctly identified the locations of star formation activity in complex molecular clouds and the spectral profiles reveal the dominant velocity components and may identify the presence of outflows.
WOS关键词	DARK ; EXCITATION
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	IOP PUBLISHING LTD
WOS记录号	WOS:000463537200010
内容类型	期刊论文
源URL	[http://libir.pmo.ac.cn/handle/332002/24496]
专题	中国科学院紫金山天文台
通讯作者	Komesh, Toktarkhan
作者单位	1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 2.Al Farabi Kazakh Natl Univ, Fac Phys & Technol, Dept Solid State Phys & Nonlinear Phys, Alma Ata 050040, Kazakhstan 3.Univ Chinese Acad Sci, Beijing 100080, Peoples R China 4.Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Peoples R China 5.ASTRON, Netherlands Inst Radio Astron, NL-7991 PD Dwingeloo, Netherlands
推荐引用方式 GB/T 7714	Komesh, Toktarkhan,Esimbek, Jarken,Baan, Willem,et al. H2CO and H110 alpha Observations toward the Aquila Molecular Cloud[J]. ASTROPHYSICAL JOURNAL,2019,874(2):10.
APA	Komesh, Toktarkhan.,Esimbek, Jarken.,Baan, Willem.,Zhou, Jianjun.,Li, Dalei.,...&Manapbayeva, Arailym.(2019).H2CO and H110 alpha Observations toward the Aquila Molecular Cloud.ASTROPHYSICAL JOURNAL,874(2),10.
MLA	Komesh, Toktarkhan,et al."H2CO and H110 alpha Observations toward the Aquila Molecular Cloud".ASTROPHYSICAL JOURNAL 874.2(2019):10.