51 Peg b revisited with VLT/CRIRES+. Constraints on atmospheric thermal structure, chemical composition, and an alternative orbital solution
D. Cont, L. Nortmann, F. Lesjak, U. Seemann, L. D. Nielsen, B. Wechselberger, F. Yan, S. Liu, A. Reiners, A. Lavail, D. Shulyak, A. Hatzes, N. Piskunov, L. Boldt-Christmas, S. Czesla, E. W. Guenther, O. Kochukhov, T. Marquart, E. Nagel, A. D. Rains, M. Rengel
astro-ph.EP
Submitted: 2026-05-22
Comments: Accepted for publication in A&A
Code: https://github.com/exoclime/FastChem
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- On the robustness of exoplanet atmospheric detections: insights from extensive simulations
- Locked In Ice: how Pebble Drift and Volatile Entrapment can Significantly Impact Carbon and Oxygen Ratios in Evolving Protoplanetary Discs
Related papers
- PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation
- Two-stage disruption of resonant chains
- Detectability of resolved hydrogen lines from the accretion shock at gas giants and their CPDs
- Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function
- Atmospheric escape fractionates secondary but not primary atmospheres
- The Occurrence Rate of Nearby Planetary Companions to Hot Jupiters