The Cygnus Allscale Survey of Chemistry and Dynamical Environments: CASCADE III. The large scale distribution of DCO+, DNC and DCN in the DR21 filament
I. Barlach Christensen, F. Wyrowski, V. S. Veena, H. Beuther, D., Semenov, K. M. Menten, A. M. Jacob, W.-J. Kim, N. Cunningham, C. Gieser, A., Hacar, S. Li, N. Schneider, I. Skretas, J. M. Winters

TL;DR
This study maps the large-scale distribution of deuterated molecules DCO+, DNC, and DCN in the DR21 filament, revealing morphological differences, anti-correlations with temperature, and potential as tracers for physical conditions in star-forming regions.
Contribution
It provides the first large-scale spatial analysis of deuterated molecules in the Cygnus-X region, highlighting their distribution, relationships, and implications for physical diagnostics.
Findings
DCO+ is the most extended deuterated molecule in the region.
Deuteration ratios are around 0.01 for DNC and DCN, and 0.005 for DCO+.
Anti-correlations exist between deuteration ratios and dust temperature or N(H2).
Abstract
Deuterated molecules and their molecular D/H-ratios (RD(D)) are important diagnostic tools to study the physical conditions of star-forming regions. The degree of deuteration, RD(D), can be significantly enhanced over the elemental D/H-ratio depending on physical parameters. Within the Cygnus Allscale Survey of Chemistry and Dynamical Environments (CASCADE), we aim to explore the large-scale distribution of deuterated molecules in the nearby Cygnus-X region. We focus on the analysis of large-scale structures of deuterated molecules in the filamentary region hosting the prominent Hii region DR21 and DR21(OH). Here we discuss the HCO+, HNC and HCN molecules and their deuterated isotopologues DCO+, DNC and DCN. The spatial distributions of integrated line emissions from DCO+, DNC, and DCN reveal morphological differences. DCO+ displays the most extended emission, characterized by several…
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