arXiv (All)
open access
Impact of accretion variability on the CO emission of a disk around a very-low-mass star with JWST
Studying the structure of very-low-mass stars ($M_\star<0.2M_\odot$) protoplanetary disk is crucial to understand the formation of Earth-like planets. In this paper, we characterize the innermost regions of the disk around a known very-low-mass star, 2MASS J16053215-1933159 (J1605 hereafter), by ana
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
- Disk survey in the Serpens star-forming region: Environmental effects in nearby star-forming regions#926646
- RIOJA. Environmental Effects on Stellar Populations and Ionized Gas in a Protocluster at $z=7.88$#620743
- RIOJA. Environmental Effects on Stellar Populations and Ionized Gas in a Protocluster at $z=7.88$#619064
- Turbulence in protoplanetary disks: A systematic analysis of dust settling in 33 disks#1146325
- Self-induced edge rings in protoplanetary disks#819618
Record · ID 1050509
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