OSTI.gov
metadata only
Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-induced Disk Heating from General-relativistic Magnetohydrodynamics and Radiative Transfer
2026 — Journal Name: The Astrophysical Journal Letters Journal Issue: 2 Journal Volume: 1010
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
- Radio Emission Properties of Millisecond Pulsars#639459
- Exploring the origin of slow-rotating pulsars: Emission from STARS simulated white dwarfs#1412969
- The dawn of TeV pulsar astronomy : search and phenomenology of pulsars at very-high-energies with the H.E.S.S. telescopes and the Fermi satellite#1120292
- Pulse Signal Simulation of Pulsars#987988
- The relationship between solar and stellar tachoclines, dynamos, and spin-down#822604
Record · ID 1471211
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