Abundance ratios in the hot ISM of elliptical galaxies

2011/03/09 by A. Pipino, F. Matteucci · 1 citation
Physics and Astronomy · #Abundance (ecology) #Astronomy and Astrophysical Research #Chemical evolution #Elliptical galaxy #Galaxies: Formation, Evolution, Phenomena #Galaxy #Gamma-ray bursts and supernovae #Interstellar medium #Stellar evolution #astro-ph.CO #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201016191

11 pages, 4 figures, to appear on A&A

arxiv created 2011/03/09 · openalex publication_date 2011/04/08 · arxiv updated 2015/05/27 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. We constrain possible explanations of the theoretical Fe discrepancy in the hot interstellar medium of elliptical galaxies and simultaneously explain the [α/Fe] ratios.

Citations

• The Contribution of Population III to the Enrichment and Preheating of the Intracluster Medium
• XMM‐NewtonandChandraObservations of the Galaxy Group NGC 5044. II. Metal Abundances and Supernova Fraction
• Stellar population models of Lick indices with variable element abundance ratios
• Greatly Extended X-Ray Emission around the Elliptical Galaxy NGC 4636 Observed with [ITAL]ASCA[/ITAL]
• XMM‐NewtonObservations of NGC 507: Supersolar Metal Abundances in the Hot Interstellar Medium
• An [ITAL]XMM-Newton[/ITAL] Observation of NGC 1399 Reveals Two Phases of Hot Gas and Supersolar Abundances in the Central Regions
• The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis
• Solar System Abundances and Condensation Temperatures of the Elements
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• X-ray evidence for spectroscopic diversity of type Ia supernovae:

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