693.932 PEOPLE
| People | Locations | Statistics |
|---|---|---|
| Naji, M. |
| |
| Motta, Antonella |
| |
| Aletan, Dirar |
| |
| Mohamed, Tarek |
| |
| Ertürk, Emre |
| |
| Taccardi, Nicola |
| |
| Kononenko, Denys |
| |
| Petrov, R. H. | Madrid |
|
| Alshaaer, Mazen | Brussels |
|
| Bih, L. |
| |
| Casati, R. |
| |
| Muller, Hermance |
| |
| Kočí, Jan | Prague |
|
| Šuljagić, Marija |
| |
| Kalteremidou, Kalliopi-Artemi | Brussels |
|
| Azam, Siraj |
| |
| Ospanova, Alyiya |
| |
| Blanpain, Bart |
| |
| Ali, M. A. |
| |
| Popa, V. |
| |
| Rančić, M. |
| |
| Ollier, Nadège |
| |
| Azevedo, Nuno Monteiro |
| |
| Landes, Michael |
| |
| Rignanese, Gian-Marco |
|
Peláez, Ramón J.
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (7/7 displayed)
- 2024Experimental Phase Function and Degree of Linear Polarization of Light Scattered by Hydrogenated Amorphous Carbon Circumstellar Dust Analogscitations
- 2019Desorption of volatile molecules from the surface of interstellar carbonaceous dust analogs
- 2018Stability of CH<sub>3</sub>NCO in Astronomical Ices under Energetic Processing: A Laboratory Studycitations
- 2018Plasma generation and processing of interstellar carbonaceous dust analogscitations
- 2017Formation of nitrile species on Ag nanostructures supported on a-Al2O3: a new corrosion route for silver exposed to the atmospherecitations
- 2012Relevance and formation mechanisms of negative ions upon ablation of Al 2O 3citations
- 2011Selective gold nanoparticles formation by pulsed laser interference.citations
Places of action
| Organizations | Location | People |
|---|
article
Desorption of volatile molecules from the surface of interstellar carbonaceous dust analogs
Abstract
<jats:title>Abstract</jats:title><jats:p>The desorption of volatile molecules from dust grains in cold dense clouds is crucial for the chemical inventory in the various stages of cloud collapse. In this work we investigate the desorption of N<jats:sub>2</jats:sub>, CO, CH<jats:sub>4</jats:sub> and CO<jats:sub>2</jats:sub> from surfaces of hydrogenated amorphous carbon (HAC), which, according to IR observations, is one of the main components of interstellar dust.</jats:p>