A merger tree with microsolar mass resolution: application to γ-ray emission from subhalo population

2008/11/30 by Carlo Giocoli, C. Giocoli, Lidia Pieri +4
Medicine · Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Galaxies: Formation, Evolution, Phenomena #Gamma-ray bursts and supernovae #Medicine #Physics #Population #Resolution (logic) #astro-ph

paper · pdf · doi:10.1111/j.1365-2966.2009.14649.x

Accepted for publication by MNRAS - 12 pages, 7 figures. Text improved and comments added. Name of a author fixed

arxiv created 2009/02/18 · openalex publication_date 2009/04/24 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

In the standard scenario of structure formation galaxies reside in massive Dark Matter (DM) haloes, where baryons can shock, cool and eventually form stars. Haloes form by gravitational instability, starting from some density fluctuation

Citations

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