[EN] The desorption process of methanol in the hot cores of massive young stars is addressed in this work. The study of pure methanol ice and when it is mixed or layered with water allows a better understanding of the physical and chemical processes which could have occurred during the formation of methanol and it is possible to infer the range of temperatures within which methanol can be found in the gas phase in these scenarios. The goal of this study was to model the desorption process of methanol as pure ice and mixed or layered with water under the conditions present in the early stages of hot cores whichcharacterize young star formation. The simulations of desorption of methanol, when it stands alone, performed in this work were compa...
Context. Methanol is a common component of interstellar and circumstellar ice mantles and is often u...
International audienceContext. Astrophysical observations show complex organic molecules (COMs) in t...
International audienceContext. Methanol, one of the simplest complex organic molecules in the inters...
The evaporation of icy mantles, which have been formed on the surface of dust grains, is acknowledge...
Interstellar methanol is only formed efficiently from hydrogenation of CO molecules accreted onto gr...
The relevance of interstellar ice to the chemical complexity of the interstellar medium has dramatic...
Context. Methanol is formed via surface reactions on icy dust grains. Methanol is also detected in t...
International audienceCold cores are an early step of star formation, characterized by densities > 1...
Aims: The gas-phase abundance of methanol in dark quiescent cores in the interstellar medium cannot ...
The complex circumstellar environment around the massive binary and luminous blue variable η Carinae...
Previous radio observations revealed widespread gas-phase methanol (CH_3OH) in the Central Molecular...
Context. Methanol is the most complex molecule that is securely identified in interstellar ices. It ...
Virtual meetingInternational audienceI. Introduction Ices throughout the ISM are exposed to differen...
Context. Methanol, one of the simplest complex organic molecules in the interstellar medium, has bee...
Context. Methanol is a common component of interstellar and circumstellar ice mantles and is often u...
International audienceContext. Astrophysical observations show complex organic molecules (COMs) in t...
International audienceContext. Methanol, one of the simplest complex organic molecules in the inters...
The evaporation of icy mantles, which have been formed on the surface of dust grains, is acknowledge...
Interstellar methanol is only formed efficiently from hydrogenation of CO molecules accreted onto gr...
The relevance of interstellar ice to the chemical complexity of the interstellar medium has dramatic...
Context. Methanol is formed via surface reactions on icy dust grains. Methanol is also detected in t...
International audienceCold cores are an early step of star formation, characterized by densities > 1...
Aims: The gas-phase abundance of methanol in dark quiescent cores in the interstellar medium cannot ...
The complex circumstellar environment around the massive binary and luminous blue variable η Carinae...
Previous radio observations revealed widespread gas-phase methanol (CH_3OH) in the Central Molecular...
Context. Methanol is the most complex molecule that is securely identified in interstellar ices. It ...
Virtual meetingInternational audienceI. Introduction Ices throughout the ISM are exposed to differen...
Context. Methanol, one of the simplest complex organic molecules in the interstellar medium, has bee...
Context. Methanol is a common component of interstellar and circumstellar ice mantles and is often u...
International audienceContext. Astrophysical observations show complex organic molecules (COMs) in t...
International audienceContext. Methanol, one of the simplest complex organic molecules in the inters...