Published on:
8 August 2023
Primary Category:
Earth and Planetary Astrophysics
Paper Authors:
Bibiana Prinoth,
H. Jens Hoeijmakers,
Stefan Pelletier,
Daniel Kitzmann,
Brett M. Morris,
Andreas Seifahrt,
David Kasper,
Heidi H. Korhonen,
Madeleine Burheim,
Jacob L. Bean,
Björn Benneke,
Nicholas W. Borsato,
Madison Brady,
Simon L. Grimm,
Rafael Luque,
Julian Stürmer,
Brian Thorsbro
Combines 8 transit observations with HARPS, HARPS-N, ESPRESSO & MAROON-X
Detects 17 species including first Sr, Sr+ & Ba+, confirms TiO
Studies signal evolution during transit using time-resolved spectroscopy
Finds signatures of ionization, dissociation & atmospheric dynamics
Atmospheric dynamics and chemistry of ultra-hot Jupiter WASP-189 b
This paper presents a combined analysis of eight transit observations of the ultra-hot Jupiter WASP-189 b using high-resolution spectroscopy. It detects 17 chemical species in the planet's atmosphere, including first detections of Sr, Sr+ and Ba+, and confirms TiO. By studying how the absorption signals change over the course of the transit as different regions rotate into view, the authors find evidence for ionization, dissociation and atmospheric dynamics shaping the transmission spectrum.
Atmospheric Clues Unlocked in Exoplanet WASP-4b
Atmospheric monitoring of ultra-hot Jupiter WASP-76b
Detection of supersonic jet and temperature differences between equatorial regions and poles of e...
Thermal properties of ultra-hot Jupiter WASP-121b
Evidence for rotation and a dense core in the hot Jupiter WASP-19Ab
Unveiling the secrets of exoplanet atmospheres through high-resolution spectroscopy
No comments yet, be the first to start the conversation...
Sign up to comment on this paper