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Table · dataset · 2025

DCO+ and DCN 1-0 survey in cold clumps

Listed in IVOA Registry (Virtual Observatory)

Deuterated molecules can be used to study the physical conditions and the astro-chemical evolution of molecular clouds.

Description

Large-sample surveys for deuterated molecules are needed to understand the enhancement of deuterated molecules from diffuse molecular gas to cold cores. A single-pointing survey toward the 559 Planck cold clumps of the Early Cold Core Catalogue (ECC) has been 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 H^13^CO+ and H^13^CN 1-0 simultaneously, aiming to determine the deuterated fraction (D_frac). Additionally, 250 cores were observed for DCO+, DCN, H^13^CO+ and H^13^CN 1-0 simultaneously. Among the 309 sources, DCO+ and DCN 1-0 were detected in 79 and 11 sources, with a detection rates of 25.6% and 3.6% respectively.

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In the 250 sources observed for all four species, DCO+, DCN, H^13^CO+ and H^13^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 D_frac(HCO+) values in 112 sources range from 0.89% to 7.4% with a median value of 3.1%, while D_frac_(HCN) values in 11 sources range from 1.5% to 5.5% with a median value of 2.3%. The line widths of DCO+ and H^13^CO+ 1-0 detections are mostly within 1km/s.

The similarity in D_frac 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, rather than during the cold core formation stage.

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