Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 317, Issue 3, Pages 563-568Publisher
BLACKWELL SCIENCE LTD
DOI: 10.1046/j.1365-8711.2000.03618.x
Keywords
molecular processes; ISM : abundances; ISM : clouds; ISM : molecules
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The possibility of nitrogen isotopic fractionation owing to ion-molecule exchange reactions involving the most abundant N-containing species in dense interstellar clouds has been explored. We find that exchange reactions between N atoms and N-containing ions have most influence on the fractionation, although the extent of fractionation is too small to be readily detectable.
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