Searching for the origin of the Ehrenreich effect in ultra-hot Jupiters. Evidence for strong C/O gradients in the atmosphere of WASP-76 b?

Sánchez-López, A.; Landman, R.; Mollière, P.; Casasayas Barris, N.; Kesseli, A.Y.; Snellen, I.A.G.

doi:10.1051/0004-6361/202142591

Searching for the origin of the Ehrenreich effect in ultra-hot Jupiters. Evidence for strong C/O gradients in the atmosphere of WASP-76 b?

Author(s):: Sánchez-López, A.; Landman, R. (0000-0002-7261-8083); Mollière, P.; Casasayas Barris, N.; Kesseli, A.Y.; Snellen, I.A.G. (0000-0003-1624-3667)

Published: 2022
Publication type: Article / Letter to editor

planets and satellitesatmospheres, planets and satellitesgaseous planets, techniquesspectroscopic, planets and satellitesindividualWASP-76 b, infraredplanetary systems, Astrophysics - Earth and Planetary Astrophysics

Date issued: 2022
Language: English
Is part of: Astronomy & Astrophysics (2022), Vol. 661, p. A78
hdl: 1887/3515522
doi: 10.1051/0004-6361/202142591
URL: https://ui.adsabs.harvard.edu/abs/2022A&A...661A..78S

Searching for the origin of the Ehrenreich effect in ultra-hot Jupiters. Evidence for strong C/O gradients in the atmosphere of WASP-76 b?

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