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51 Peg b revisited with VLT/CRIRES+

So far, the majority of high-resolution spectroscopy studies on exoplanet atmospheres have focused on transiting planetary systems. Consequently, the atmospheres of non-transiting exoplanets remain poorly explored, and the potential of high-resolution spectroscopy for determining key planetary param...

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Autors principals: Cont D., Nortmann L., Lesjak F., Seemann U., Nielsen L. D., Wechselberger B., Yan F., Liu S., Reiners A., Lavail A., Shulyak D., Hatzes A., Piskunov N., Boldt-Christmas L., Czesla S., Guenther E. W., Kochukhov O., Marquart T., Nagel E., Rains A. D., Rengel M.
Format: Artigo
Idioma:Inglês
Publicat: EDP Sciences 2026-06-01
Col·lecció:Astronomy & Astrophysics
Matèries:
techniques: spectroscopic
planets and satellites: atmospheres
planets and satellites: individual: 51 peg b
Accés en línia:https://www.aanda.org/articles/aa/full_html/2026/06/aa58116-25/aa58116-25.html
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