The Metallicity and Carbon-to-oxygen Ratio of the Ultrahot Jupiter WASP-76b from Gemini-S/IGRINS
Measurements of the carbon-to-oxygen (C/O) ratios of exoplanet atmospheres can reveal details about their formation and evolution. Recently, high-resolution cross-correlation analysis has emerged as a method of precisely constraining the C/O ratios of hot Jupiter atmospheres. We present two transits...
Κύριοι συγγραφείς: | Weiner Mansfield, M, Line, MR, Wardenier, JP, Brogi, M, Bean, JL, Beltz, H, Smith, P, Zalesky, JA, Batalha, N, Kempton, EM, Montet, BT, Owen, JE, Plavchan, P, Rauscher, E |
---|---|
Μορφή: | Journal article |
Γλώσσα: | English |
Έκδοση: |
IOP Publishing
2024
|
Παρόμοια τεκμήρια
Παρόμοια τεκμήρια
-
The Metallicity and Carbon-to-oxygen Ratio of the Ultrahot Jupiter WASP-76b from Gemini-S/IGRINS
ανά: Megan Weiner Mansfield, κ.ά.
Έκδοση: (2024-01-01) -
The Roasting Marshmallows Program with IGRINS on Gemini South I: Composition and Climate of the Ultrahot Jupiter WASP-18 b
ανά: Matteo Brogi, κ.ά.
Έκδοση: (2023-01-01) -
Magnetic Effects and 3D Structure in Theoretical High-resolution Transmission Spectra of Ultrahot Jupiters: the Case of WASP-76b
ανά: Hayley Beltz, κ.ά.
Έκδοση: (2023-01-01) -
Up, Up, and Away: Winds and Dynamical Structure as a Function of Altitude in the Ultrahot Jupiter WASP-76b
ανά: Aurora Y. Kesseli, κ.ά.
Έκδοση: (2024-01-01) -
The Roasting Marshmallows Program with IGRINS on Gemini South. II. WASP-121 b has Superstellar C/O and Refractory-to-volatile Ratios
ανά: Peter C. B. Smith, κ.ά.
Έκδοση: (2024-01-01)