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Including a luminous central remnant in radiative transfer simulations for Type Iax supernovae
Callan, F. P. (Corresponding author) ; Sim, S. A. ; Collins, C.GSI* ; Shingles, L. J.GSI* ; Lach, F. ; Röpke, F. K. ; Pakmor, R. ; Kromer, M. ; Srivastav, S.
2024
Oxford Univ. Press
Oxford
This record in other databases: 
Please use a persistent id in citations: doi:10.1093/mnras/stae847 doi:10.15120/GSI-2024-00853
Note: This is an Open Access article distributed under the terms of the Creative Commons Attribution License ( https:// creativecommons.org/ licenses/ by/ 4.0/ )
Contributing Institute(s):
- Nukleare Astrophysik & Struktur (KNA)
Research Program(s):
- 612 - Cosmic Matter in the Laboratory (POF4-612) (POF4-612)
- HEAVYMETAL - How Neutron Star Mergers make Heavy Elements (101071865) (101071865)
- KILONOVA - Probing r-process nucleosynthesis through its electromagnetic signatures (885281) (885281)
- DFG project 279384907 - SFB 1245: Atomkerne: Von fundamentalen Wechselwirkungen zu Struktur und Sternen (279384907) (279384907)
- ChETEC-INFRA - Chemical Elements as Tracers of the Evolution of the Cosmos - Infrastructures for Nuclear Astrophysics (101008324) (101008324)
Experiment(s):
- no experiment theory work (theory)
Appears in the scientific report
2024
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