Inferring the star-formation histories of the most massive and passive early-type galaxies atz< 0.3
2016/04/26 by Annalisa Citro, Lucia Pozzetti, L. Pozzetti +4 · 67 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Extinction (optical mineralogy) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy formation and evolution #Halo #Metallicity #Physics #Redshift #Star formation #Stars #Stellar, planetary, and galactic studies #astro-ph.GA
paper · pdf · doi:10.1051/0004-6361/201527772
published in Astronomy and Astrophysics 592, A19 (EDP Sciences) · 25 pages, 25 figures, 4 tables. Accepted for publication in Astronomy & Astrophysics
arxiv created 2016/04/26 · openalex publication_date 2016/05/18 · openalex created_date 2016/06/24 · arxiv updated 2016/07/13 · openalex updated_date 2026/08/05
Abstract
Context. In the Λ cold dark matter (ΛCDM) cosmological framework, massive galaxies are the end-points of the hierarchical evolution and are therefore key probes for understanding how the baryonic matter evolves within the dark matter halos.
Citations
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