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 |
|
Hirashita, H.
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (5/5 displayed)
- 2024Radial properties of dust in galaxies: Comparison between observations and isolated galaxy simulationscitations
- 2022Dust grain size evolution in local galaxies: a comparison between observations and simulationscitations
- 2022Dust grain size evolution in local galaxies : a comparison between observations and simulationscitations
- 2003Dust and Hydrogen Molecules in Metal-Poor Galaxies
- 2002A Far-Infrared SED Model of Extremely Young Low Metallicity Galaxies
Places of action
| Organizations | Location | People |
|---|
document
Dust and Hydrogen Molecules in Metal-Poor Galaxies
Abstract
In order to understand the chemical and thermodynamical state of the interstellar medium (ISM) in the early stage of galaxy evolution, dust formation needs to be considered. Even in metal poor galaxies, dust grains can drastically accelerate the formation rate of molecular hydrogen (H[2]). Hydrogen molecules emit vibrational-rotational lines, thus cooling the gas. Consequently, the abundance of the molecules affects the spectrum and the cooling rate of a galaxy....