TiO and VO broad band absorption features in the optical spectrum of the atmosphere of the hot-Jupiter HD 209458b

2008/09/10 by J. -M. Desert, Jean-Michel Désert, A. Vidal‐Madjar +9 · 1 citation
Physics and Astronomy · #Astro and Planetary Science #Astronomy and Astrophysical Research #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:200810355

9 pages, 4 figures. Accepted for publication in Astronomy & Astrophysics

arxiv created 2008/09/10 · openalex publication_date 2008/10/27 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Aims. The presence of titanium oxide (TiO) and vanadium oxide (VO) gas phase species is searched for in the atmosphere of the hot Jupiter HD 209458b.

Citations

• A Possible Bifurcation in Atmospheres of Strongly Irradiated Stars and Planets
• The Influence of Atmospheric Dynamics on the Infrared Spectra and Light Curves of Hot Jupiters
• Atomic data for resonance absorption lines. I - Wavelengths longward of the Lyman limit
• New Spectral Types L and T
• Detection of Thermal Emission from an Extrasolar Planet

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• Exoplanet Atmospheres