Effects of the radial inflow of gas and galactic fountains on the chemical evolution of M 31

2013/01/22 by E. Spitoni, F. Matteuccí, F. Matteucci +1 · 36 citations
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Chemical evolution #Galactic Center #Galaxies: Formation, Evolution, Phenomena #Galaxy #Physics #RADIUS #Star formation #Stellar, planetary, and galactic studies #astro-ph.CO #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201220401

published in Astronomy and Astrophysics 551, A123 (EDP Sciences) · Accepted by A&A

arxiv created 2013/01/22 · openalex publication_date 2013/02/11 · arxiv updated 2013/03/13 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context. Galactic fountains and radial gas flows are very important ingredients for modeling the chemical evolution of galactic disks.

Citations

• Investigating the Andromeda stream — I. Simple analytic bulge—disc—halo model for M31
• The Flattened Dark Matter Halo of M31 as Deduced from the Observed HiScale Heights
• Galactic hydrostatic equilibrium with magnetic tension and cosmic-ray diffusion
• Darwin Tames an Andromeda Dwarf: Unraveling the Orbit of NGC 205 Using a Genetic Algorithm
• Abundance Gradients and the Formation of the Milky Way
• Radial Variation of Attenuation and Star Formation in the Largest Late‐Type Disks Observed with GALEX
• The chemical evolution of a Milky Way-like galaxy: the importance of a cosmologically motivated infall law
• Chemical evolution with radial mixing
• Contrasting the chemical evolution of the Milky Way and Andromeda
• Chemical evolution and the galactic habitable zone of M31 (the Andromeda Galaxy)
• PROBING THE INTERGALACTIC MEDIUM/GALAXY CONNECTION. V. ON THE ORIGIN OF Lyα AND O VI ABSORPTION ATz< 0.2

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