Double tail structure in escaping atmospheres of magnetised close-in planets
- Author(s)
- A. A. Vidotto, S. Carolan, Gopal Hazra, Carolina Villarreal D'Angelo, D. Kubyshkina
- Abstract
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(s)
- Department of Astrophysics
- External organisation(s)
- Leiden University, Trinity College London, Instituto de Astronomía Teórica y Experimental, Österreichische Akademie der Wissenschaften (ÖAW)
- Volume
- 17
- Pages
- 232-234
- No. of pages
- 3
- DOI
- https://doi.org/10.1017/S1743921323000340
- Publication date
- 08-2023
- Peer reviewed
- Yes
- Austrian Fields of Science 2012
- 103004 Astrophysics
- Keywords
- ASJC Scopus subject areas
- Astronomy and Astrophysics, Space and Planetary Science
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/663b81ca-0ba3-4fd7-afe9-fbd80a041b1f