Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 693905.0, MPI für Astronomie / Publikationen_mpia
New extended deuterium fractionation model: assessment at dense ISM conditions and sensitivity analysis
Authors:Albertsson, T.; Semenov, D. A.; Vasyunin, A. I.; Henning, T.; Herbst, E.
Date of Publication (YYYY-MM-DD):2013
Title of Journal:The Astrophysical Journal Supplement Series
Volume:207
Issue / Number:2
Start Page:id. 27 (29 pp)
Audience:Not Specified
Abstract / Description:Observations of deuterated species are useful in probing the temperature, ionization level, evolutionary stage, chemistry, and thermal history of astrophysical environments. The analysis of data from the Atacama Large Millimeter Array and other new telescopes requires an elaborate model of deuterium fractionation. This paper presents a publicly available chemical network with multi-deuterated species and an extended, up-to-date set of gas-phase and surface reactions. To test this network, we simulate deuterium fractionation in diverse interstellar sources. Two cases of initial abundances are considered: (1) atomic except for H2 and HD, and (2) molecular from a prestellar core. We reproduce the observed D/H ratios of many deuterated molecules, and sort the species according to their sensitivity to temperature gradients and initial abundances. We find that many multiply deuterated species produced at 10 K retain enhanced D/H ratios at temperatures <~ 100 K. We study how recent updates to reaction rates affect calculated D/H ratios, and perform a detailed sensitivity analysis of the uncertainties of the gas-phase reaction rates in the network. We find that uncertainties are generally lower in dark cloud environments than in warm infrared dark clouds and that uncertainties increase with the size of the molecule and number of D-atoms. A set of the most problematic reactions is presented. We list potentially observable deuterated species predicted to be abundant in low- and high-mass star-formation regions.
Free Keywords:astrochemistry; circumstellar matter; ISM: clouds; ISM: molecules; methods: numerical; molecular processes; stars: protostars
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:ISSN:0067-0049 %R 10.1088/0067-0049/207/2/27
URL:http://cdsads.u-strasbg.fr/abs/2013ApJS..207...27A
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.