arXiv (All)
open access
Systematic and Statistical Properties of Prominence Eruptions on the M-dwarf YZ CMi
M-dwarfs produce frequent flares, and their associated mass ejections are expected to significantly affect the habitability of close-in exoplanets. Recent spectroscopic observations have revealed several prominence eruptions-indicative of stellar mass ejections-on M-dwarfs through Doppler shifts of
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
- Systematic and Statistical Properties of Prominence Eruptions on the M-dwarf YZ CMi#921012
- Improved Constraints on the Surface of LHS 3844 b from its Mid-Infrared Spectrum#1142284
- K-dwarf starspot hunters: how to directly characterize spot and faculae properties with UV-IR panchromatic transit spectra#1130328
- Impact of accretion variability on the CO emission of a disk around a very-low-mass star with JWST#1050509
- Characterizing Stellar Flares in Ariel Targets: Activity Analysis and Transit Contamination#620701
Record · ID 925248
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