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...

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Detalles Bibliográficos
Publicado:	2018
Materias:	galaxies: abundances galaxies: evolution galaxies: high-redshift infrared: galaxies
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v869_n1_p_DeRossi http://hdl.handle.net/20.500.12110/paper_0004637X_v869_n1_p_DeRossi
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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