Double tail structure in escaping atmospheres of magnetised close-in planets

Autor(en)
A. A. Vidotto, S. Carolan, Gopal Hazra, Carolina Villarreal D'Angelo, D. Kubyshkina
Abstrakt

High-energy stellar irradiation can photoevaporate planetary atmospheres, which can be observed in spectroscopic transits of hydrogen lines. Here, we investigate the effect of planetary magnetic fields on the observational signatures of atmospheric escape in hot Jupiters.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Leiden University, Trinity College London, Instituto de Astronomía Teórica y Experimental, Österreichische Akademie der Wissenschaften (ÖAW)
Band
17
Seiten
232-234
Anzahl der Seiten
3
DOI
https://doi.org/10.1017/S1743921323000340
Publikationsdatum
08-2023
Peer-reviewed
Ja
ÖFOS 2012
103004 Astrophysik
Schlagwörter
ASJC Scopus Sachgebiete
Astronomy and Astrophysics, Space and Planetary Science
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/663b81ca-0ba3-4fd7-afe9-fbd80a041b1f