arXiv (All)
open access
SN 2024afyu interpreted as a Pair Instability Supernova
Pair-instability supernovae (PISNe) are the predicted explosions of very massive stars triggered by electron-positron pair production. Numerous transients have been proposed as PISN candidates, yet none has provided unambiguous confirmation of this explosion mechanism. The predicted strengths of neb
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Molecular bipolar outflow in SN 1987A supports the jittering-jets explosion mechanism#1011047
- The Destruction of the Circumstellar Ring of Sn 1987a#643647
- First measurements of N-subjettiness in central Pb-Pb collisions at sNN = 2.76 TeV#491842
- GRMHD Simulations of Accreting Proto-Magnetars II. Implications for r-process Nucleosynthesis#819655
- GRMHD Simulations of Accreting Proto-Magnetars II. Implications for r-process Nucleosynthesis#809659
Record · ID 985338
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive