Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Ben Drummond"'
Autor:
Vivien Parmentier, Nathan J. Mayne, Stefan Lines, Thomas Mikal-Evans, Ian A. Boutle, David K. Sing, Duncan Christie, James Manners, Ben Drummond, Krisztian Kohary
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 506:4500-4515
We present results of 3D hydrodynamical simulations of HD209458b including a coupled, radiatively-active cloud model ({\sc EddySed}). We investigate the role of the mixing by replacing the default convective treatment used in previous works with a mo
Autor:
Stefan Lines, Nathan J. Mayne, David K. Sing, Ben Drummond, Krisztian Kohary, James Manners, Ian A. Boutle, Thomas Mikal-Evans
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 488:1332-1355
We present results from 3D radiative-hydrodynamical simulations of HD 209458b with a fully coupled treatment of clouds using the EddySed code, critically, including cloud radiative feedback via absorption and scattering. We demonstrate that the therm
Thermal dissociation and recombination of molecular hydrogen, H_2, in the atmospheres of ultra-hot Jupiters (UHJs) has been shown to play an important role in global heat redistribution. This, in turn, significantly impacts their planetary emission,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e591e641a84c5f1e34307e438735b6b9
http://arxiv.org/abs/2104.14376
http://arxiv.org/abs/2104.14376
Autor:
Ben Drummond, Mark W. Phillips, Eric Hébrard, Jayesh M. Goyal, Isabelle Baraffe, Nicole F. Allard, Fernand Spiegelman, Pascal Tremblin, Gilles Chabrier
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 637, pp.A38. ⟨10.1051/0004-6361/201937381⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 637, pp.A38. ⟨10.1051/0004-6361/201937381⟩
Astronomy and Astrophysics-A&A, 2020, 637, pp.A38. ⟨10.1051/0004-6361/201937381⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 637, pp.A38. ⟨10.1051/0004-6361/201937381⟩
We present a new set of solar metallicity atmosphere and evolutionary models for very cool brown dwarfs and self-luminous giant exoplanets, which we term ATMO 2020. Atmosphere models are generated with our state-of-the-art 1D radiative-convective equ