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. We suggest that the enhancement of DCO<sup>+<sup/> and DCN likely begins in the early diffuse stage of the molecular cloud and not during the cold-core formation stage.","PeriodicalId":8571,"journal":{"name":"Astronomy & Astrophysics","volume":"39 1","pages":""},"PeriodicalIF":5.8000,"publicationDate":"2025-04-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"DCO+ and DCN 1–0 survey toward a sample of Planck cold clumps\",\"authors\":\"Fu Mo, Junzhi Wang, Shu Liu, Yan Duan, Huanxue Feng, Yuqiang Li, Zhe Lu, Rui Luo, Chao Ou, Yani Xu, Zhuoying Yan\",\"doi\":\"10.1051/0004-6361/202452072\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<i>Context.<i/> Deuterated molecules can be used to study the physical conditions and astro-chemical evolution of molecular clouds.<i>Aims.<i/> Large-sample surveys for deuterated molecules are needed to understand the enhancement of deuterated molecules from diffuse molecular gas to cold cores.<i>Methods.<i/> 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 <i>J<i/> = 1–0 transitions of DCO<sup>+<sup/> and DCN. 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. We suggest that the enhancement of DCO<sup>+<sup/> and DCN likely begins in the early diffuse stage of the molecular cloud and not during the cold-core formation stage.\",\"PeriodicalId\":8571,\"journal\":{\"name\":\"Astronomy & Astrophysics\",\"volume\":\"39 1\",\"pages\":\"\"},\"PeriodicalIF\":5.8000,\"publicationDate\":\"2025-04-11\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Astronomy & Astrophysics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1051/0004-6361/202452072\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomy & Astrophysics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1051/0004-6361/202452072","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
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.
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.