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...
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 |
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Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
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Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acd339 |
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