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Hα and He λ10830 Spectrum of WASP-52b by stas810200 is a document available to read on EtoBox.

What is Hα and He λ10830 Spectrum of WASP-52b about?

This study models the Hα and He λ10830 transmission spectra of the exoplanet WASP-52b, utilizing a hydrodynamic model and Monte Carlo simulations to analyze atmospheric properties. The findings indicate that a high H/He ratio and specific X-ray and extreme-ultraviolet flux conditions are necessary to fit the observations, with a mass-loss rate estimated at 2.8 × 10^11 g s−1. The research highlights the importance of simultaneous modeling of these spectral lines to better understand exoplanetary atmospheres.

Author

stas810200

Language

EN