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.
Links
Where it is published
- Reference page cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/696/A140 ↗
landing page · from IVOA Registry
Documentation and papers
- ADS 2025A&A...696A.140M ui.adsabs.harvard.edu/abs/2025A%26A...696A.140M ↗
publication · from IVOA Registry
Catalogue records · 2
- VOResource record dc.g-vo.org/oai.xml?verb=GetRecord&metadataPrefix=ivo_vor&identifier=ivo%3… ↗
metadata API · from IVOA Registry
- Registry record (GAVO) dc.g-vo.org/I/cds.vizier/j/a%2Ba/696/a140 ↗
catalogue entry · from IVOA Registry
Topics
- Stated by source
- Radio
- From keywords
- Astronomy & Astrophysics
- Inferred from text
- Astronomical sciences 68%
Provenance · 1 source records, 9 field assertions
| Source | Key | Last seen | Raw |
|---|---|---|---|
| IVOA Registry (Virtual Observatory) | ivo://cds.vizier/j/a+a/696/a140 | 13 d ago | JSON v1 |
| Field | Assertion | Extractor | Evidence |
|---|---|---|---|
| access_level | source · IVOA Registry | connector:ivoa_registry@1.0.0 | |
| concepts[field].anzsrc:group:5101 | enrichment · IVOA Registry | taxonomy-embedding@1.1.0 | title+keywords+description (68%) |
| concepts[field].local:field:astronomy | mapping · IVOA Registry | connector:ivoa_registry@1.0.0 | |
| concepts[modality].ivoa_waveband:radio | source · IVOA Registry | connector:ivoa_registry@1.0.0 | |
| description | source · IVOA Registry | connector:ivoa_registry@1.0.0 | rr.resource.res_description |
| license_text | source · IVOA Registry | connector:ivoa_registry@1.0.0 | |
| publication_date | source · IVOA Registry | connector:ivoa_registry@1.0.0 | |
| title | source · IVOA Registry | connector:ivoa_registry@1.0.0 | rr.resource.res_title |
| updated_date | source · IVOA Registry | connector:ivoa_registry@1.0.0 |