International audienceMeasurements using the Far Ultraviolet Spectroscopic Explorer (FUSE) show that the gas-phase D/H ratio in the solar neighborhood is highly variable and suggest that the elemental abundance of deuterium in the Galactic disk may be higher than previously thought. We investigate in this Letter the possible consequences of such an enhanced D/H ratio on the deuterium fractionation in singly and multiply deuterated molecules in cold, dense gas. We show that a modest increase in the elemental abundance of deuterium can lead to significant enhancements in abundances of multiply deuterated species
Observations of CH3D in the atmospheres of the outer planets provide a test of the theory of deuteri...
International audienceWe present column density measurements of the HD molecule in the interstellar ...
Since the detection of unexpectedly high deuterium fractionation in the Galactic Center almost 20 ye...
International audienceMeasurements using the Far Ultraviolet Spectroscopic Explorer (FUSE) show that...
19 pages, 9 figuresAnalyses of spectra obtained with the Far Ultraviolet Spectroscopic Explorer (FUS...
International audienceAnalyses of spectra obtained with the Far Ultraviolet Spectroscopic Explorer (...
A survey of the abundances of deuterium in planetary atmospheres and small bodies has been carried o...
In this Letter, we present the first results from updated models of interstellar deuterium chemistry...
Author Institution: Department of Physics, The Ohio State University; Departments of Physics, Astron...
The abundance ratio of D:H in the interstellar medium can be derived either more directly from the U...
Observations of low mass protostars which probe small enough size scales to be within likely CO depl...
The tendency for deuterium to be concentrated into the cold dense regions of the galaxy is due to t...
Aims.In a recently published 1-millimeter line survey of the Orion Bar by Leurini et al., the confir...
Estimates of the interstellar deuterium abundance span a wide range of values. Until recently, it wa...
The D/H ratio in interstellar gas varies on scales of a few hundred pc in the local Milky Way, with ...
Observations of CH3D in the atmospheres of the outer planets provide a test of the theory of deuteri...
International audienceWe present column density measurements of the HD molecule in the interstellar ...
Since the detection of unexpectedly high deuterium fractionation in the Galactic Center almost 20 ye...
International audienceMeasurements using the Far Ultraviolet Spectroscopic Explorer (FUSE) show that...
19 pages, 9 figuresAnalyses of spectra obtained with the Far Ultraviolet Spectroscopic Explorer (FUS...
International audienceAnalyses of spectra obtained with the Far Ultraviolet Spectroscopic Explorer (...
A survey of the abundances of deuterium in planetary atmospheres and small bodies has been carried o...
In this Letter, we present the first results from updated models of interstellar deuterium chemistry...
Author Institution: Department of Physics, The Ohio State University; Departments of Physics, Astron...
The abundance ratio of D:H in the interstellar medium can be derived either more directly from the U...
Observations of low mass protostars which probe small enough size scales to be within likely CO depl...
The tendency for deuterium to be concentrated into the cold dense regions of the galaxy is due to t...
Aims.In a recently published 1-millimeter line survey of the Orion Bar by Leurini et al., the confir...
Estimates of the interstellar deuterium abundance span a wide range of values. Until recently, it wa...
The D/H ratio in interstellar gas varies on scales of a few hundred pc in the local Milky Way, with ...
Observations of CH3D in the atmospheres of the outer planets provide a test of the theory of deuteri...
International audienceWe present column density measurements of the HD molecule in the interstellar ...
Since the detection of unexpectedly high deuterium fractionation in the Galactic Center almost 20 ye...