arXiv (All)
open access
XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
GX 5-1 is one of the brightest persistent neutron-star low-mass X-ray binaries in the Galaxy and one of the classical Z sources accreting at luminosities close to or above the Eddington limit. We present the first high-resolution X-ray spectroscopic study of GX 5-1 with the Resolve micro-calorimeter
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
- Long-term X-ray spectral analysis of Cygnus X-1 using AstroSat#1000045
- Revealing the accretion disc structure in Changing State AGN: NGC1566#1142923
- X-ray measurements of the elemental abundances for the diffuse emission in the nuclear starburst galaxy NGC 3079#1141959
- Energy-Resolved Limits on Orbital X-ray Polarization Modulation in Cygnus X-1#1070861
- Fundamental differences in the X-ray accretion properties of low and high-excitation radio galaxies#926998
Record · ID 1145009
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