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| Naji, M. |
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| Mohamed, Tarek |
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| Ertürk, Emre |
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| Taccardi, Nicola |
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| Petrov, R. H. | Madrid |
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| Casati, R. |
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| Azevedo, Nuno Monteiro |
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Ferrara, A.
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Publications (8/8 displayed)
- 2022The ALMA REBELS survey: the dust content of z 7 Lyman break galaxiescitations
- 2019Microstructural Evolution and Steam Oxidation Resistance of Field-tested Thor (tm) 115 Steel
- 2017The impact of chemistry on the structure of high-z galaxiescitations
- 2004Dust formation in very massive primordial supernovaecitations
- 2003Dust and Hydrogen Molecules in Metal-Poor Galaxies
- 2003Dust and Hydrogen Molecules in Metal-Poor Galaxies
- 2002A Far-Infrared SED Model of Extremely Young Low Metallicity Galaxies
- 2002A Far-Infrared SED Model of Extremely Young Low Metallicity Galaxies
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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....