Revisiting the Perseus Cluster III: Role of Aspherical Explosions on its Chemical Composition and Extension to Metal-Poor Stars and Galaxies

Abstract

The Perseus Cluster has been precisely measured by the legacy Hitomi telescope on the Si-group (Si, S, Ar, Ca) and Fe-group elements (Cr, Mn, Ni). These element abundance ratios provide insight into the typical behaviour of supernovae. In Paper II, we presented new massive star explosion models at various metallicity, assuming spherical explosions. We show that while the fitting is improved, some features (e.g., Ni/Fe) remain to be improved. In this article, we extend our calculation to an aspherical explosion using the jet-induced explosion mechanism. The detailed pre- and post-explosion chemical profiles are calculated with a large post-processing network to capture the production of odd-number elements (V, Mn, Cu) and iron-group elements. We further explore how the jet-driven explosions create the diversity of models which could be compatible with the observed diversity in terms of ${}^{56}$Ni-mass vs ejecta mass, Ti-V relation, and stellar abundances. Finally, we apply the new collapsar models in the Galactic Chemical Evolution context. We study how the galactic stars, including the Zn-enriched star HE 1327-2326, can put constraints on the relative rates of collapsar and some of its model parameters. We show that collapsar could lead to significant changes in some elements, e.g., Zn. Our study shows that the collapsar is a necessary component to explain multiple elemental trends observed in the Milky Way Galaxy.

arXiv comment23 pages, 39 figures. Submitted to the Astrophysical Journal on Nov 10 2025, revised on Feb 5 2026, accepted on Feb 7 2026, published on Apr 7 2026

References in corpus (63)

• Array Programming with NumPy
• Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
• The Zwicky Transient Facility: System Overview, Performance, and First Results
• Discovery of the peculiar supernova 1998bw in the error box of GRB980425
• The Nucleosynthetic Signature of Population III
• First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
• Galactic Chemical Evolution: Hydrogen Through Zinc
• Theory of Core-Collapse Supernovae
• A `Hypernova' model for SN 1998bw associated with gamma-ray burst of 25 April 1998
• Nucleosynthesis of Zinc and Iron-Peak Elements in Pop III Type II Supernovae : Comparison with abundances of Very Metal-Poor Halo Stars
• A Search for Stars of Very Low Metal Abundance. VI. Detailed Abundances of 313 Metal-Poor Stars
• Relativistic Jets in Collapsars
• The Stellar Abundances for Galactic Archeology (SAGA) Database - Compilation of the Characteristics of Known Extremely Metal-Poor Stars
• Explosive yields of massive stars from Z=0 to Z=Zsun
• Asymmetric Supernovae, Pulsars, Magnetars, and Gamma-Ray Bursts
• Jet-Induced Explosions of Core Collapse Supernovae
• Supernova Nucleosynthesis in Population III 13 -- 50 $M_{\odot }$ Stars and Abundance Patterns of Extremely Metal-Poor Stars
• Gamma-Ray Bursts and Type Ic Supernovae: SN 1998bw
• The Propagation and Eruption of Relativistic Jets from the Stellar Progenitors of GRBs
• Sub-Chandrasekhar-mass white dwarf detonations revisited
• A complete sample of bright Swift Long Gamma-Ray Bursts: Sample presentation, Luminosity Function and evolution
• Hydrodynamics of core-collapse supernovae and their progenitors
• The optically unbiased GRB host (TOUGH) survey. I. Survey design and catalogs
• The Swift GRB Host Galaxy Legacy Survey - II. Rest-Frame NIR Luminosity Distribution and Evidence for a Near-Solar Metallicity Threshold
• Type Ia Supernovae as Sites of p-process: Two-Dimensional Models Coupled to Nucleosynthesis
• Explosive Nucleosynthesis in Hypernovae
• New Hubble Space Telescope Observations of Heavy Elements in Four Metal-Poor Stars
• Aspherical Explosion Models for SN 1998bw/GRB 980425
• Light curves of hydrogen-poor Superluminous Supernovae from the Palomar Transient Factory
• Explosive Nucleosynthesis in Near-Chandrasekhar Mass White Dwarf Models for Type Ia Supernovae: Dependence on Model Parameters
• Explosive Nucleosynthesis in Axisymmetrically Deformed Type II Supernovae
• Aspherical Properties of Hydrodynamics and Nucleosynthesis in Jet-induced Supernovae
• Analysis of broad-lined Type Ic supernovae from the (intermediate) Palomar Transient Factory
• Explosive Nucleosynthesis in Sub-Chandrasekhar Mass White Dwarf Models for Type Ia Supernovae: Dependence on Model Parameters
• Evidence for an aspherical Population III supernova explosion inferred from the hyper metal-poor star HE1327-2326
• Constraints on the Chemical Enrichment History of the Perseus Cluster of Galaxies from High-Resolution X-ray Spectroscopy
• Evidence for Sub-Chandrasekhar Type Ia Supernovae from Stellar Abundances in Dwarf Galaxies
• Evolution of ONeMg Core in Super-AGB Stars towards Electron-Capture Supernovae: Effects of Updated Electron-Capture Rate
• Electron Capture Supernovae of Super-AGB Stars: Sensitivity on Input Physics
• Matter Mixing in Axisymmetric Supernova Explosion
• Luminous Supernovae: Unveiling a Population Between Superluminous and Normal Core-collapse Supernovae
• Explosive Nucleosynthesis in GRB Jets Accompanied by Hypernovae
• A new hydrodynamics code for Type Ia Supernovae
• Explosive Nucleosynthesis Associated with Formation of Jet-induced GRBs in Massive Stars
• The chemical signature of jet-driven hypernovae
• The distribution of [$\alpha$/Fe] in the Milky Way disc
• Collapsar R-Process Yields Can Reproduce [Eu/Fe] Abundance Scatter in Metal-Poor Stars
• Supernovae, Pulsars and Gamma-Ray Bursts: A Unified Picture
• Dark Matter Admixed Type Ia Supernovae
• Machine learning detects multiplicity of the first stars in stellar archaeology data
• Chemical abundances in the outskirts of nearby galaxy groups measured with joint Suzaku and Chandra observations
• Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- I: Formation of Low-mass Neutron Stars
• Origin of metals in old Milky Way halo stars based on GALAH and Gaia
• Non-parametric Morphologies of Mergers in the Illustris Simulation
• Search for Extremely Metal-Poor Stars with GEMINI-N/GRACES I. Chemical-Abundance Analysis
• The metallicity and star formation activity of long gamma-ray burst hosts for z$<$3: insights from the Illustris simulation
• Hypernova Nucleosynthesis and Galactic Chemical Evolution
• Hydrodynamics and Nucleosynthesis of Jet-Driven Supernovae I: Parameter Study of the Dependence on Jet Energetics
• Metallicity-Suppressed Collapsars Cannot be the Dominant r-Process Source in the Milky Way
• Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- II: Rotation and Gravitational-wave Signals
• Hydrodynamics and Nucleosynthesis of Jet-Driven Supernovae II: Comparisons with Abundances of Extremely Metal-Poor Galaxies and Constraints on Supernova Progenitors
• Revisiting the Perseus Cluster I: Resolving the Si/S/Ar/Ca ratios by Stellar Convection
• Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History