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arXiv · 2405.17717

X-ray Irradiation of the Giant Planet Orbiting the T Tauri Star TAP 26

Stephen L. Skinner·Manuel Guedel
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Abstract

We present new Chandra X-ray observations of TAP 26, a ~17 Myr old magnetically-active weak-lined T Tauri star that has been reported to host a massive planet in a 10.8 day orbit. At a separation of a = 0.097 AU the planet will be exposed to intense X-ray and UV radiation from the star. The first observation caught the star in a state of elevated X-ray emission with variability on a timescale of a few hours and an X-ray temperature kTx ~ 2 - 4 keV. Two subsequent observations 5-10 days later showed slow variability and a lower X-ray flux and temperature (kTx ~ 1 keV). We characterize the X-ray emission and estimate the X-ray ionization and heating rates that will need to be incorporated into realistic models of the planet's atmosphere.

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Stephen L. Skinner, Manuel Guedel. 2024-05-28. X-ray Irradiation of the Giant Planet Orbiting the T Tauri Star TAP 26. https://arxiv.org/abs/2405.17717

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