X-Ray and Ultraviolet Emission of the Young Planet-hosting Star V1298 Tau from Coordinated Observations with XMM-Newton and Hubble Space Telescope

X-Ray and Ultraviolet Emission of the Young Planet-hosting Star V1298 Tau from Coordinated Observations with XMM-Newton and Hubble Space Telescope

Atmospheric mass loss plays a major role in the evolution of exoplanets. This process is driven by the stellar high-energy irradiation, especially in the first hundreds of millions of years after dissipation of the proto-planetary disk. A major source of uncertainty in modeling atmospheric photoevap...

Full description

Bibliographic Details
Main Authors: A. Maggio, I. Pillitteri, C. Argiroffi, S. Benatti, J. Sanz-Forcada, V. D’Orazi, K. Biazzo, F. Borsa, L. Cabona, R. Claudi, S. Desidera, D. Locci, D. Nardiello, L. Mancini, G. Micela, M. Rainer, R. Spinelli, A. Bignamini, M. Damasso
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Single x-ray stars
Ultraviolet spectroscopy
Star-planet interactions
Stellar activity
Pre-main sequence stars
Extreme ultraviolet astronomy
Online Access:https://doi.org/10.3847/1538-4357/acd339

Internet

https://doi.org/10.3847/1538-4357/acd339

Similar Items