arXiv (All)
open access
Merger remnant in TXS 1033+026 - I: $\rm Hα$ and HI 21-cm observations suggest counter-rotating gas
We have conducted eMERLIN and GEMINI IFU observations towards TXS 1033+026, a post-merger ultraluminous infrared galaxy, to study the radio continuum, $\rm Hα$ and HI 21-cm lines at sub-kpc scales. We find a symmetric, two-sided core-jet structure in both L ($\approx 1.4$ GHz)- and C ($\approx 4.8$
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 impact of relativistic AGN jets on realistic galaxy cluster environments#1155412
- Jet--ISM Interactions in Gaseous Disks: Simulating Kinetic Feedback in the Radio Galaxy 3C 326 N#1123153
- Slow stellar halo rotation as a signature of disc flips and GES-like mergers#984249
- A ${}^{13}$CO Detection in a Massive Molecular Gas Flow in Abell 1795's Central Galaxy#1356868
- Electromagnetic flares from compact-object mergers in active galactic nucleus disks: Signatures and predictions#449048
Record · ID 1187978
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