Evidence of energy-, recombination-, and photon-limited escape regimes in giant planet H/He atmospheres

Autor: Pedro J. Amado, Manuel López-Puertas, Luisa Lara, Jose A. Caballero, Enric Palle, M. Salz, Jorge Sanz-Forcada, Ignasi Ribas, Th. Henning, Ansgar Reiners, Lisa Nortmann, Andreas Quirrenbach, D. Montes, M. Lampón, S. Czesla, A. Sánchez-López, Karan Molaverdikhani

Publikováno v: E-Prints Complutense. Archivo Institucional de la UCM
instname
Astronomy & Astrophysics, 648, 1-9
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Astronomy & Astrophysics
Manuel López-Puertas
Digital.CSIC. Repositorio Institucional del CSIC

Hydrodynamic escape is the most efficient atmospheric mechanism of planetary mass loss and has a large impact on planetary evolution. Three hydrodynamic escape regimes have been identified theoretically: energy-limited, recombination-limited, and pho

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::50259322ae19fd3b6c17ee958517f389
http://arxiv.org/abs/2104.08832

Discriminating between hazy and clear hot-Jupiter atmospheres with CARMENES

Autor: Manuel López-Puertas, M. R. Zapatero Osorio, Lev Tal-Or, Mathias Zechmeister, Enric Palle, Víctor J. S. Béjar, Karan Molaverdikhani, Th. Henning, Lisa Nortmann, Andreas Quirrenbach, S. Czesla, J. Aceituno, P. J. Amado, Ansgar Reiners, F. F. Bauer, A. Sánchez-López, M. Stangret, J. A. Caballero, Ignas Snellen, Núria Casasayas-Barris, Evangelos Nagel, D. Montes, Ignasi Ribas

Publikováno v: Astronomy & Astrophysics, 643, A24
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy & Astrophysics
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid

Context. Relatively large radii of some hot Jupiters observed in the ultraviolet and blue-optical are generally interpreted to be due to Rayleigh scattering by high-altitude haze particles. However, the haze composition and its production mechanisms

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7c116ad21d2952bf1e94583b5fb155e8
http://hdl.handle.net/1887/3133910

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Exoplanet atmospheres with GIANO. I. Water in the transmission spectrum of HD 189 733 b

Autor: Aldo S. Bonomo, Luigi Mancini, G. Guilluy, Paolo Giacobbe, R. de Kok, Matteo Brogi, Alessandro Sozzetti

Publikováno v: Astronomy and Astrophysics, 615, A16
Astronomy and Astrophysics 615 (2018)
Astronomy and Astrophysics, 615. EDP Sciences
Astronomy and Astrophysics
Astronomy and Astrophysics, 615

High-resolution spectroscopy (R $\ge$ 20,000) at near-infrared wavelengths can be used to investigate the composition, structure, and circulation patterns of exoplanet atmospheres. However, up to now it has been the exclusive dominion of the biggest

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::66f7aa265f42806449579d0254bce988
https://ui.adsabs.harvard.edu/#abs/2018A&A...615A..16B

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