DCO+和DCN 1-0对普朗克冷团块样本的调查

IF 5.8 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Fu Mo, Junzhi Wang, Shu Liu, Yan Duan, Huanxue Feng, Yuqiang Li, Zhe Lu, Rui Luo, Chao Ou, Yani Xu, Zhuoying Yan
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The survey included observations of 309 cores for DCO<sup>+<sup/> and DCN 1–0 simultaneously, followed by 71 of these cores where DCO<sup>+<sup/> 1–0 was detected for H<sup>13<sup/>CO<sup>+<sup/> and H<sup>13<sup/>CN 1–0 simultaneously, aiming to determine the deuterated fraction (<i>D<i/><sub>frac<sub/>). Additionally, 250 cores were observed for DCO<sup>+<sup/>, DCN, H<sup>13<sup/>CO<sup>+<sup/>, and H<sup>13<sup/>CN 1–0 simultaneously.<i>Results.<i/> DCO<sup>+<sup/> and DCN 1–0 were detected in 79 and 11 of the 309 sources, with detection rates of 25.6% and 3.6%, respectively. In the 250 sources that were observed for all four species, DCO<sup>+<sup/>, DCN, H<sup>13<sup/>CO<sup>+<sup/>, and H<sup>13<sup/>CN 1–0 were detected in 58, 9, 57, and 13 sources, with a detection rate of 23.2%, 3.6%, 22.8%, and 5.2%, respectively. The <i>D<i/><sub>frac<sub/>(HCO<sup>+<sup/>) values in 112 sources range from 0.89% to 7.4%, with a median value of 3.1%, while <i>D<i/><sub>frac<sub/>(HCN) values in 11 sources range from 1.5% to 5.5%, with a median value of 2.3%. The line widths of the DCO<sup>+<sup/> and H<sup>13<sup/>CO<sup>+<sup/> 1–0 detections are mostly within 1 km s<sup>−1<sup/>.<i>Conclusions.<i/> The similarity in <i>D<i/><sub>frac<sub/> values between HCO+ and HCN indicates that the higher detection rate of DCO<sup>+<sup/> 1–0 compared with DCN 1–0 is due to the lower critical density of DCO<sup>+<sup/> 1–0. 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引用次数: 0

摘要

上下文。氘化分子可用于研究分子云的物理条件和天体化学演化。需要对氘化分子进行大样本调查,以了解氘化分子从弥漫分子气体到冷核的增强。利用亚利桑那射电天文台12米望远镜对早期冷核目录(ECC)中的559个普朗克冷团进行了单点调查,重点关注DCO+和DCN的J = 1-0跃迁。在309个岩心中同时检测到DCO+和DCN 1-0,在其中71个岩心中同时检测到H13CO+和H13CN 1-0的DCO+ 1-0,目的是确定氘化分数(Dfrac)。此外,250个核同时观察了DCO+、DCN、H13CO+和H13CN 1-0。309个源中有79个源检测到DCO+, 11个源检测到DCN 1-0,检出率分别为25.6%和3.6%。在共250个源中,检测到DCO+、DCN、H13CO+和H13CN 1-0的源分别为58个、9个、57个和13个,检出率分别为23.2%、3.6%、22.8%和5.2%。112个源的Dfrac(HCO+)值在0.89% ~ 7.4%之间,中位数为3.1%;11个源的Dfrac(HCN)值在1.5% ~ 5.5%之间,中位数为2.3%。DCO+和H13CO+ 1 - 0检测线宽多在1 km s−1以内。HCO+和HCN的Dfrac值相似,说明DCO+ 1-0的检出率高于DCN 1-0是由于DCO+ 1-0的临界密度较低。我们认为DCO+和DCN的增强可能始于分子云的早期扩散阶段,而不是在冷核形成阶段。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
DCO+ and DCN 1–0 survey toward a sample of Planck cold clumps
Context. Deuterated molecules can be used to study the physical conditions and astro-chemical evolution of molecular clouds.Aims. Large-sample surveys for deuterated molecules are needed to understand the enhancement of deuterated molecules from diffuse molecular gas to cold cores.Methods. A single-pointing survey toward the 559 Planck cold clumps of the Early Cold Core Catalogue (ECC) was conducted using the Arizona Radio Observatory 12-meter telescope, focusing on the J = 1–0 transitions of DCO+ and DCN. The survey included observations of 309 cores for DCO+ and DCN 1–0 simultaneously, followed by 71 of these cores where DCO+ 1–0 was detected for H13CO+ and H13CN 1–0 simultaneously, aiming to determine the deuterated fraction (Dfrac). Additionally, 250 cores were observed for DCO+, DCN, H13CO+, and H13CN 1–0 simultaneously.Results. DCO+ and DCN 1–0 were detected in 79 and 11 of the 309 sources, with detection rates of 25.6% and 3.6%, respectively. In the 250 sources that were observed for all four species, DCO+, DCN, H13CO+, and H13CN 1–0 were detected in 58, 9, 57, and 13 sources, with a detection rate of 23.2%, 3.6%, 22.8%, and 5.2%, respectively. The Dfrac(HCO+) values in 112 sources range from 0.89% to 7.4%, with a median value of 3.1%, while Dfrac(HCN) values in 11 sources range from 1.5% to 5.5%, with a median value of 2.3%. The line widths of the DCO+ and H13CO+ 1–0 detections are mostly within 1 km s−1.Conclusions. The similarity in Dfrac values between HCO+ and HCN indicates that the higher detection rate of DCO+ 1–0 compared with DCN 1–0 is due to the lower critical density of DCO+ 1–0. We suggest that the enhancement of DCO+ and DCN likely begins in the early diffuse stage of the molecular cloud and not during the cold-core formation stage.
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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