arXiv (All)
open access
Relativistic effects of PSR~J1856--0039 double neutron star system in a 2.36-hour compact orbit
Compact double neutron star (DNS) systems are unique laboratories for testing gravitational theories and studying DNS mergers. Here we report the properties of a new DNS system, PSR J1856--0039, discovered in the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The pulsar is mildly recy
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
- First study of the 6-neutron system from the decay of resonances in ¹⁰He#350676
- Vertical time-of-flight spectroscopy of ultracold neutrons#391911
- Exploring the formation mechanisms of double neutron star systems: an analytical perspective#364407
- Rotating Radio Transient Phases of Isolated Neutron Star Systems and Descendants of Central Compact Objects#1050467
Record · ID 1012289
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