Gaseous SiO and Silicate Clouds in Three Benchmark Early-L Dwarfs

arXiv:2610.11530 · astro-ph.SR, astro-ph.EP · Submitted 2026-10-08 · Read on arXiv

astro-ph.SR, astro-ph.EP

Submitted: 2026-10-08

Updated: 2026-10-08

Terminology

• Abundance — 15× in this paper · explained in 1 episode
• Benchmark — 8× in this paper · explained in 2 episodes
• Metallicity — 5× in this paper · explained in 3 episodes
• Calibration — 3× in this paper · explained in 7 episodes
• Degeneracy — 3× in this paper · explained in 3 episodes
• Trace — 2× in this paper · explained in 2 episodes
• Core — 1× in this paper · explained in 2 episodes
• Mikulski Archive for Space Telescopes — 1× in this paper
• Robustness — 1× in this paper · explained in 5 episodes

Sources

• Silicate Clouds, SiO, and Molecular Trends across the L-T Sequence: A JWST/MIRI LRS Spectral Library of Brown Dwarfs
• Benchmark Brown Dwarf Systems I: Chemical Abundance Analysis of FGK Stars with Wide-Separation Brown Dwarf Companions Using PEPSI
• The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems VIII: patchy forsterite and enstatite clouds in the atmosphere of VHS 1256 b, retrieval lessons learned and outlook to the future

Related papers

• HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager
• Effect of Neutron Star Jets on Common Envelope Evolution
• Constraining the origin of magnetic white dwarfs
• JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting
• Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics
• Can MHD Oscillations Modulate Quasi-Periodic Plasma Release from Coronal Streamers?