3D model of hydrogen atmospheric escape from HD 209458b and HD 189733b: radiative blow-out and stellar wind interactions
Atmospheric escape from HD 189733b observed in H I Lyman-a: detailed analysis of HST/STIS September 2011 observations
Disentangling Stellar and Airglow Emission Lines from Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS) Spectra
Fluctuations and Flares in the Ultraviolet Line Emission of Cool Stars: Implications for Exoplanet Transit Observations
Hubble Space Telescope detection of oxygen in the atmosphere of exoplanet HD 189733b
Hydrodynamic Atmospheric Escape in HD 189733 b: Signatures of Carbon and Hydrogen Measured with the Hubble Space Telescope
Modeling the Lya transit absorption of the hot Jupiter HD 189733b
Modelling the He I triplet absorption at 10 830 A in the atmospheres of HD 189733 b and GJ 3470 b
MOVES III. Simultaneous X-ray and ultraviolet observations unveiling the variable environment of the hot Jupiter HD 189733b
MOVES - IV. Modelling the influence of stellar XUV-flux, cosmic rays, and stellar energetic particles on the atmospheric composition of the hot Jupiter HD 189733b
Near-ultraviolet Absorption, Chromospheric Activity, and Star-Planet Interactions in the WASP-12 system
Nonthermal Motions and Atmospheric Heating of Cool Stars
Temporal variations in the evaporating atmosphere of the exoplanet HD 189733b
The Influence of the Extreme Ultraviolet Spectral Energy Distribution on the Structure and Composition of the Upper Atmosphere of Exoplanets
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Lecavelier des Etangs et al., 2012, 'Dynamics in the atmosphere of the evaporating planet HD189733b', 1.0, European Space Agency, https://doi.org/10.5270/esa-8zq5dzy