arXiv (All)
open access
TOI-3686: A Hot Jupiter and Sub-Neptune In A 2:1 Mean-Motion Resonance
Hot Jupiters are typically thought to be "lonely", but a small and growing subset of them have been found to have nearby planets in the same system. We present the discovery of a new member of this class of systems, TOI-3686. TOI-3686 c is a hot Jupiter with $P_\mathrm{orb} = 5.078$ days detected by
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 the Planetary Obliquity Distribution of Warm Jupiters#821620
- Uncovering the rapidly evolving orbits of the dynamic TOI-201 system#1066225
- Revisiting TOI-4438 and TOI-442 planetary systems with new observations from SPIRou and TESS#1366949
- ISO far-infrared observations of rich galaxy clusters II. Sersic 159-03#639553
- KMT-2026-BLG-0083L: A Two-Jovian-Planet System Orbiting an M Dwarf Discovered by Microlensing#1000399
Record · ID 1412592
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