The Far-infrared Emission of the First Massive Galaxies
Massive Population II galaxies undergoing the first phase of vigorous star formation after the initial Population III stage should have high energy densities and silicate-rich interstellar dust. We have modeled the resulting far-infrared spectral energy distributions (SEDs), demonstrating that they...
| Autores principales: | De Rossi, M.E., Rieke, G.H., Shivaei, I., Bromm, V., Lyu, J. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v869_n1_p_DeRossi |
| Aporte de: |
Ejemplares similares
-
The Far-infrared Emission of the First Massive Galaxies
Publicado: (2018) -
The evolution of galaxy metallicity scaling relations in cosmological hydrodynamical simulations
por: De Rossi, M.E., et al. -
Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level
por: De Rossi, M.E., et al. -
The evolution of galaxy metallicity scaling relations in cosmological hydrodynamical simulations
Publicado: (2015) -
A bias in optical observations of high-redshift luminous infrared galaxies
Publicado: (2004)