arXiv (All)
open access
Direct imaging of sub-parsec binary SMBHs in the central galaxy of the NGC 5044 group
Binary active galactic nuclei (AGN) consist of two supermassive black holes (SMBHs) hosted in a single galaxy that are simultaneously accreting gas. These systems are key to understanding hierarchical galaxy evolution and represent prime targets for low-frequency gravitational wave (GW) experiments.
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
- Constraining AGN Disk Properties with Gravitational Waves from Inspiraling Stellar-Mass Binary Black Holes in Hierarchical Triple Systems#820941
- Combining Direct Black Hole Mass Measurements and Spatially Resolved Stellar Kinematics to Calibrate the MBH–σ⋆ Relation of Active Galaxies#982798
- Potential binary supermassive black holes in Markarian 231 as a scientific case for the spectropolarimeter POLLUX#1077405
- A New Sample of $\sim$ 100 Intermediate-mass Black Holes Reaching $z \approx 1$#984729
- ALMA CO(2-1) Gas Dynamics in NGC 315: A Multi-Method Benchmark for Supermassive Black Hole Mass Measurement#819048
Record · ID 1037116
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