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Observations of interstellar HNC, DNC, and HN/sup 13/C: Temperature effects on deuterium fractionation

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/156900· OSTI ID:6251411
We report here an extensive search for DNC emission in 18 clouds with HNC emission. The DNC molecule was found in 13 of these clouds. The HN/sup 13/C molecule was also sought in those clouds where saturation was thought to be important. We have determined the (DNC)/(HNC) ratios incorporating the effects of saturation and radiation trapping. The extent of deuteration found in HNC is larger than for any other molecule yet observed. The (DNC)/(HNC) ratios are also found to strongly anticorrelate with the kinetic temperature of the cloud, suggesting that exchange reactions between HD and a molecular ion are ultimately responsible for the deuteration. The value of ..delta..E/k for the exchange reaction that produces DNC is determined to be 240 +- 60 K. Low values for the abundance of electrons and certain neutral species are similar to those determined from (DCO/sup +/)/(HCO/sup +/) and (N/sub 2/D/sup +/)/(N/sub 2/H/sup +/).
Research Organization:
Department of Astronomy and Electrical Engineering Research Laboratory, University of Texas at Austin
OSTI ID:
6251411
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 228:3; ISSN ASJOA
Country of Publication:
United States
Language:
English