A possibly solar metallicity atmosphere escaping from HAT-P-32b revealed by Hα and He absorption

This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Bibliographic Details
Authors: Yan, Dongdong, Guo, Jianheng, Seon, Kwang-il, López-Puertas, Manuel, Czesla, Stefan, Lampón, M., Van Eck, S.
Format: article
Status:Published version
Publication Date:2024
Country:España
Institution:Consejo Superior de Investigaciones Científicas (CSIC)
Repository:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/369505
Online Access:http://hdl.handle.net/10261/369505
Access Level:Open access
Keyword:Hydrodynamics
Radiative transfer
Methods: numerical
Planets and satellites: atmospheres
Planets and satellites: composition
Planets and satellites: individual: HAT-P-32b
Description
Summary:This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

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