arXiv (All)
open access
Exploring the origin of slow-rotating pulsars: Emission from STARS simulated white dwarfs
An increasing number of slow-rotating pulsars and long-period transients have been observed in recent years. The periods of these sources can be significantly longer than typical pulsar sources, ranging from ~ 100 - 1000 s, or even longer. The observed periods and period derivatives predict high mag
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 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
- Radio Emission Properties of Millisecond Pulsars#639459
- Intrinsic versus observation induced spin nonstationarity in pulsar timing#1157326
- Discovery of Hidden Extragalactic Pulsars in the Parkes Archival Data#1249874
- Tentative rotation in a galaxy at z ~ 14 with ALMA#1065832
Record · ID 1412969
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