The Relative Supernovae Contribution to the Chemical Enrichment History of Abell 1837

Abstract

In this paper, we report the relative SNe contributions on the metal budget of the ICM of Abell 1837 galaxy cluster at redshift z $=$ 0.069. For this purpose, we analysed the hot ICM of the cluster and obtained radial metal distributions by using XMM-Newton archival data with total exposure $\sim$100 ks. These metal measurements consist of Mg, Si, S, Fe and Ni within 0.7 R${}_{500}$ radius which is divided into three concentric annuli. In order to explain the observed metal abundance pattern in terms of relative supernova contributions, we used our newly developed code SNeRatio which utilizes theoretical nucleosynthesis models. This study covers the most recent 3D SNIa and SNcc yield tables. All combinations of these theoretical yields were fitted with our measured abundance ratios and statistically acceptable ones were selected. Each of these models were found to predict a uniform SNIa percentage contribution to the total SNe from the cluster center to the outskirts and form an SNIa ratio distribution with a mean 39 $\pm$ 14$\%$. This uniformity is consistent with the early enrichment scenario which assumes that the metal production processes begin in early phase of cluster formation, namely proto-cluster phase at epoch z $\ge$ 2.

arXiv comment9 pages, 6 figures. Accepted for publication in Monthly Notices of the Royal Astronomical Society. For associated source files, see https://github.com/kiyami/sneratio

References in corpus (51)

• The chemical composition of the Sun
• Cosmic Star Formation History
• Collisional Plasma Models with APEC/APED: Emission Line Diagnostics of Hydrogen-like and Helium-like Ions
• HI4PI: A full-sky HI survey based on EBHIS and GASS
• Heating Hot Atmospheres with Active Galactic Nuclei
• Astrophysics Source Code Library
• SparsePak: A Formatted Fiber Field Unit for The WIYN Telescope Bench Spectrograph. I. Design, Construction, and Calibration
• A very deep Chandra observation of the Perseus cluster: shocks, ripples and conduction
• Updated Atomic Data and Calculations for X-ray Spectroscopy
• Three-dimensional delayed-detonation models with nucleosynthesis for Type Ia supernovae
• An investigation of cooling flows and general cluster properties from an X-ray image deprojection analysis of 207 clusters of galaxies
• The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton
• A Catalog of Galaxy Clusters Observed by XMM-Newton
• Three-dimensional pure deflagration models with nucleosynthesis and synthetic observables for Type Ia supernovae
• Chandra Observation of the Radio Source / X-ray Gas Interaction in the Cooling Flow Cluster Abell 2052
• Discovery of Ghost Cavities in Abell 2597's X-ray Atmosphere
• X-Ray Evidence for Multiphase Hot Gas with Nearly Solar Fe Abundances in the Brightest Groups of Galaxies
• A uniform metal distribution in the intergalactic medium of the Perseus cluster of galaxies
• On the role of AGN feedback on the thermal and chemodynamical properties of the hot intra-cluster medium
• An ASCA Study of the Heavy Element Distribution in Clusters of Galaxies
• Chemical enrichment in the cluster of galaxies Hydra A
• Geometrical Evidence for Dark Matter: X-ray Constraints on the Mass of the Elliptical Galaxy NGC 720
• Constraining supernova models using the hot gas in clusters of galaxies
• Temperature and entropy profiles of nearby cooling flow clusters observed with XMM-Newton
• The elemental abundances in the intracluster medium as observed with XMM-Newton
• Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi
• Radial metal abundance profiles in the intra-cluster medium of cool-core galaxy clusters, groups, and ellipticals
• Temperature and Heavy Element Abundance Profiles of Cool Clusters of Galaxies from ASCA
• Solar abundance ratios of the iron-peak elements in the Perseus Cluster
• Implications of the central metal abundance peak in cooling core clusters of galaxies
• The history of chemical enrichment in the intracluster medium from cosmological simulations
• A uniform metallicity in the outskirts of massive, nearby galaxy clusters
• XMM-Newton Spectroscopy of the Cluster of Galaxies 2A 0335+096
• Chemical evolution in Sersic 159-03 observed with XMM-Newton
• The Athena space X-ray Observatory and the astrophysics of hot plasma
• The origin of ICM enrichment in the outskirts of present-day galaxy clusters from cosmological hydrodynamical simulations
• Temperature and abundance profiles of hot gas in galaxy groups - II. Implications for feedback and ICM enrichment
• A Uniform Contribution of Core-Collapse and Type Ia Supernovae to the Chemical Enrichment Pattern in the Outskirts of the Virgo Cluster
• The Non-Uniformity of Galaxy Cluster Metallicity Profiles
• Constraints on the Chemical Enrichment History of the Perseus Cluster of Galaxies from High-Resolution X-ray Spectroscopy
• Origin of central abundances in the hot intra-cluster medium - II. Chemical enrichment and supernova yield models
• Origin of central abundances in the hot intra-cluster medium - I. Individual and average abundance ratios from XMM-Newton EPIC
• CHEERS: The chemical evolution RGS sample
• High Resolution XMM-Newton Spectroscopy of the Cooling Flow Cluster A3112
• Abundance and temperature distributions in the hot intra-cluster gas of Abell 4059
• Athena X-IFU synthetic observations of galaxy clusters to probe the chemical enrichment of the Universe
• Solar chemical composition in the hot gas of cool-core ellipticals, groups, and clusters of galaxies
• Uniform Contribution of Supernova Explosions to the Chemical Enrichment of Abell 3112 out to R200
• Suzaku Observations of Metal Distributions in the Intracluster Medium of the Centaurus Cluster
• Constraining the origin and models of chemical enrichment in galaxy clusters using the Athena X-IFU
• A High Spectral Resolution Study of the Soft X-ray Background with the X-ray Quantum Calorimeter

Cited by in corpus (5)

• Chemical enrichment in the cool core of the Centaurus cluster of galaxies
• Chemical enrichment of the ICM within the Virgo cluster I: radial profiles
• The infalling elliptical galaxy M89: The chemical composition of the AGN disturbed hot atmosphere
• Chemical enrichment of ICM within the A3266 cluster I: radial profiles
• Chemical Enrichment of Isolated Relic Galaxy Mrk1216