Detection of Paschen β absorption in the atmosphere of KELT-9 b: A new window into the atmospheres of ultra-hot Jupiters

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.

Detalles Bibliográficos
Autores: Sánchez-López, A., Lin, L., Snellen, I. A. G., Casasayas-Barris, N., García Muñoz, A., Lampón, M., López-Puertas, Manuel
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2022
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/295323
Acceso en línea:http://hdl.handle.net/10261/295323
Access Level:acceso abierto
Palabra clave:Planets and satellites: atmospheres
Planets and satellites: gaseous planets
Planets and satellites: individual: KELT-9 b
Descripción
Sumario: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.