arXiv (All)
open access
Post-merger rotational evolution of magnetised single hot subdwarfs results in slow rotation due to magnetic braking
Single hot subdwarfs are believed to form through mergers of helium-core white dwarfs, which can lead to large-scale magnetic fields generated during the merger, and may be observable at the surface once they evolve into the stable core-helium burning phase. As a post-merger product, the orbital ang
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
- Magnetic field morphological diagnostics with ALMA in the G327.29 protocluster: VGT versus dust polarization#1048559
- Wind-Fed Magnetic Flux and the Emergence of X-ray Coronae in Active Galactic Nuclei#1247608
- Dissecting the dust distribution and polarization around two B213 young stellar objects with ALMA#156188
- Gravitational-wave background from supermassive black holes without merger trees: Tidally regulated mergers and direct inference from the NANOGrav 15 yr data#1202639
- Two hot pre-white dwarfs inside the red giant branch planetary nebula Pa 13#413234
Record · ID 1354360
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