arXiv (All)
open access
Binary Progenitors of Electron-capture Supernovae
Electron-capture supernovae (ECSNe) arise from a narrow progenitor parameter space between oxygen-neon white dwarf formation and iron-core collapse supernovae, governed by the competition between core growth and envelope removal. Binary interactions modify this balance through mass transfer and merg
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
- The diversity of late-time interaction in Type II supernovae#1414642
- Multi-Wavelength Identification of a Luminous Mid-Infrared Supernova Powered by Circumstellar Interaction with Binary-Driven Pre-supernova Mass Loss#987259
- Direct Detection of Type II-P Supernova Progenitors with the $\textit{Euclid}$ and CSST Surveys#798730
- Direct Detection of Type II-P Supernova Progenitors with the $\textit{Euclid}$ and CSST Surveys#797316
- Early panchromatic spectra reveal helium in the thermonuclear supernova 2024kce#1423466
Record · ID 1457853
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