Detection of the hydrogen Balmer lines in the ultra-hot Jupiter WASP-33b

Author(s):
Yan, F.; Wyttenbach, A.; Casasayas-Barris, N.; Reiners, A.; Pallé, E.; Henning, T.; Mollière, P.; Czesla, S.; Nortmann, L.; Molaverdikhani, K.; Chen, G.; Snellen, I.A.G. (0000-0003-1624-3667); Zechmeister, M.; Huang, C.; Ribas, I.; Quirrenbach, A.; Caballero, J.A.; Amado, P.J.; Cont, D.; Khalafinejad, S.; Khaimova, J.; López-Puertas, M.; Montes, D.; Nagel, E.; Oshagh, M.; Pedraz, S.; Stangret, M.
Published
2021
Publication type
Article / Letter to editor
Planets and SatellitesAtmospheresTechniquesSpectroscopicIndividualWASP-33bAstrophysicsEarth and Planetary Astrophysics
Date issued
2021
Language
English
Is part of
Astronomy and Astrophysics
hdl
1887/3251009
doi
10.1051/0004-6361/202039302
URL
https://ui.adsabs.harvard.edu/abs/2021A&A...645A..22Y