Can cluster merger shocks reproduce the luminosity and shape distribution of radio relics?

Radio relics in galaxy clusters are believed to trace merger shock fronts. If cosmological structure formation determines the luminosity, size and shape distributions of radio relics, then merger shocks need to be lighted up in a homogeneous way. We investigate if a mock relic sample, obtained from...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autor principal: Nuza, Sebastián E.
Publicado: 2017
Materias:
Galaxies: clusters: general
Large-scale structure of Universe
Methods: numerical
Radiation mechanisms: non-thermal
Shock waves
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v470_n1_p240_Nuza
http://hdl.handle.net/20.500.12110/paper_00358711_v470_n1_p240_Nuza
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

Ejemplares similares