Chemistry of TMC-1 with multiply deuterated species and spin chemistry of H2, H2+, H3+ and their isotopologues
VASTEL, C.
Centre d'étude spatiale des rayonnements [CESR]
Centre d'étude spatiale des rayonnements [CESR]
< Réduire
Centre d'étude spatiale des rayonnements [CESR]
Centre d'étude spatiale des rayonnements [CESR]
Langue
en
Article de revue
Ce document a été publié dans
Monthly Notices of the Royal Astronomical Society. 2017, vol. 466, p. 4470-4479
Oxford University Press (OUP): Policy P - Oxford Open Option A
Résumé en anglais
Deuterated species are unique and powerful tools in astronomy since they can probe the physical conditions, chemistry, and ionization level of various astrophysical media. Recent observations of several deuterated species ...Lire la suite >
Deuterated species are unique and powerful tools in astronomy since they can probe the physical conditions, chemistry, and ionization level of various astrophysical media. Recent observations of several deuterated species along with some of their spin isomeric forms have rekindled the interest for more accurate studies on deuterium fractionation. This paper presents the first publicly available chemical network of multiply deuterated species along with spin chemistry implemented on the latest state-of-the-art gas-grain chemical code `NAUTILUS'. D/H ratios for all deuterated species observed at different positions of TMC-1 are compared with the results of our model, which considers multiply deuterated species along with the spin chemistry of light hydrogen bearing species H2, H2+, H3+ and their isotopologues. We also show the differences in the modeled abundances of non-deuterated species after the inclusion of deuteration and spin chemistry in the model. Finally, we present a list of potentially observable deuterated species in TMC-1 awaiting detection.< Réduire
Mots clés en anglais
Astrophysics - Astrophysics of Galaxies
Origine
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