Atmospheric mass loss and stellar wind effects in young and old systems I: comparative 3D study of TOI-942 and TOI-421 systems
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DOI: 10.1093/mnras/stab3594
Abstract: At young ages, when radiation from the host star is high, and the planet is hot and inflated after formation, planetary atmospheric mass loss can be extremely strong compared to older planets. In turn, stellar… read more here.
Keywords: toi 942; mass; atmospheric mass; 942 toi ... See more keywords