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...
المؤلفون الرئيسيون: | 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 |
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التنسيق: | Journal article |
اللغة: | English |
منشور في: |
IOP Publishing
2024
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مواد مشابهة
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The Metallicity and Carbon-to-oxygen Ratio of the Ultrahot Jupiter WASP-76b from Gemini-S/IGRINS
حسب: Megan Weiner Mansfield, وآخرون
منشور في: (2024-01-01) -
The Roasting Marshmallows Program with IGRINS on Gemini South I: Composition and Climate of the Ultrahot Jupiter WASP-18 b
حسب: Matteo Brogi, وآخرون
منشور في: (2023-01-01) -
Magnetic Effects and 3D Structure in Theoretical High-resolution Transmission Spectra of Ultrahot Jupiters: the Case of WASP-76b
حسب: Hayley Beltz, وآخرون
منشور في: (2023-01-01) -
Up, Up, and Away: Winds and Dynamical Structure as a Function of Altitude in the Ultrahot Jupiter WASP-76b
حسب: Aurora Y. Kesseli, وآخرون
منشور في: (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
حسب: Peter C. B. Smith, وآخرون
منشور في: (2024-01-01)