Chemical properties of long gamma-ray bursts progenitors in cosmological simulations

In this work, we investigate the chemical dependence of the progenitors of long gamma-ray bursts. Using hydrodynamical cosmological simulations consistent with the concordance Λ-CDM model which include star formation, chemical enrichment and supernova feedback in a self-consistent way, and assuming...

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Detalles Bibliográficos
Autores principales: Pellizza, L.J., Artale, M.C., Tissera, P.B.
Formato: CONF
Materias:
Chemical properties
Stars
Energy Observatory
Gamma ray bursts
Luminosity functions
Massive stars
Metallicities
Monte carlo schemes
Spectral peak energies
Star formations
Gamma rays
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_18248039_v2012-May_n_p_Pellizza
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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