This thesis is devoted to the study of regular and deuterated water in ices and on surfaces against an interstellar background. A large network for the formation of regular water has been studied with the use of a Kinetic Monte Carlo model. A specific reaction has been investigated as well: H2 + O -> OH + H. Furthermore, in the light of deuterium fractionation, a thermal study on deuteron scrambling in the ice has been performed: H2O + D2O -> 2 HDO. Finally, two low-temperature routes relevant to HDO formation have been investigated: H2O + OD -> OH + HDO and D2O + OH -> OD + HDO.Laboratory astrophysics and astrochemistr
Water (H2O) ice is an important solid constituent of many astrophysical environments. To comprehend ...
Recent interferometer observations have found that the D2O/HDO abundance ratio is higher than that o...
Understanding the evolution of water during star formation, from the molecular cloud down to the pro...
International audienceContext. Millimetric observations have measured high degrees of molecular deut...
Context. Millimetric observations have measured high degrees of molecular deuteration in several spe...
Water is an important oxygen reservoir in space and is often used as a tracer of large-scale gas-pha...
In the interstellar medium (ISM), an important channel of water formation is the reaction of atoms o...
The formation of interstellar water is commonly accepted to occur on the surfaces of icy dust grains...
Observations of star-forming environments revealed that the abundances of some deuterated interstell...
To date more than 170 species have been identified in interstellar space, and the chemical processes...
The HDO/H2O ratio measured in interstellar gas is often used to draw conclusions on the formation an...
We investigate the delivery of regular and deuterated forms of water from prestellar cores to circum...
International audienceWe investigate water and deuterated water chemistry in turbulent protoplanetar...
This is the author’s version of the work. It is posted here by permission of the AAAS for personal u...
The formation of interstellar water is commonly accepted to occur on the surfaces of icy dust grains...
Water (H2O) ice is an important solid constituent of many astrophysical environments. To comprehend ...
Recent interferometer observations have found that the D2O/HDO abundance ratio is higher than that o...
Understanding the evolution of water during star formation, from the molecular cloud down to the pro...
International audienceContext. Millimetric observations have measured high degrees of molecular deut...
Context. Millimetric observations have measured high degrees of molecular deuteration in several spe...
Water is an important oxygen reservoir in space and is often used as a tracer of large-scale gas-pha...
In the interstellar medium (ISM), an important channel of water formation is the reaction of atoms o...
The formation of interstellar water is commonly accepted to occur on the surfaces of icy dust grains...
Observations of star-forming environments revealed that the abundances of some deuterated interstell...
To date more than 170 species have been identified in interstellar space, and the chemical processes...
The HDO/H2O ratio measured in interstellar gas is often used to draw conclusions on the formation an...
We investigate the delivery of regular and deuterated forms of water from prestellar cores to circum...
International audienceWe investigate water and deuterated water chemistry in turbulent protoplanetar...
This is the author’s version of the work. It is posted here by permission of the AAAS for personal u...
The formation of interstellar water is commonly accepted to occur on the surfaces of icy dust grains...
Water (H2O) ice is an important solid constituent of many astrophysical environments. To comprehend ...
Recent interferometer observations have found that the D2O/HDO abundance ratio is higher than that o...
Understanding the evolution of water during star formation, from the molecular cloud down to the pro...