15NH3 in the atmosphere of a cool brown dwarf
Author:
Barrado DavidORCID, Mollière Paul, Patapis Polychronis, Min MichielORCID, Tremblin PascalORCID, Ardevol Martinez Francisco, Whiteford Niall, Vasist Malavika, Argyriou IoannisORCID, Samland Matthias, Lagage Pierre-Olivier, Decin LeenORCID, Waters RensORCID, Henning ThomasORCID, Morales-Calderón MaríaORCID, Guedel Manuel, Vandenbussche BartORCID, Absil OlivierORCID, Baudoz PierreORCID, Boccaletti Anthony, Bouwman JeroenORCID, Cossou ChristopheORCID, Coulais Alain, Crouzet NicolasORCID, Gastaud René, Glasse AlistairORCID, Glauser Adrian M.ORCID, Kamp Inga, Kendrew Sarah, Krause Oliver, Lahuis FredORCID, Mueller Michael, Olofsson Göran, Pye JohnORCID, Rouan DanielORCID, Royer PierreORCID, Scheithauer SilviaORCID, Waldmann Ingo, Colina Luis, van Dishoeck Ewine F.ORCID, Ray TomORCID, Östlin GöranORCID, Wright Gillian
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Reference66 articles.
1. Burrows, A. et al. A nongray theory of extrasolar giant planets and brown dwarfs. Astrophys. J. 491, 856–875 (1997). 2. Faherty, J. K. in Handbook of Exoplanets (eds Deeg, H. & Belmonte, J.) 531–542 (Springer, 2018). 3. Madhusudhan, N., Amin, M. A. & Kennedy, G. M. Toward chemical constraints on hot Jupiter migration. Astrophys. J. Lett. 794, L12 (2014). 4. Mollière, P. et al. Interpreting the atmospheric composition of exoplanets: sensitivity to planet formation assumptions. Astrophys. J. 934, 74 (2022). 5. Feuchtgruber, H. et al. The D/H ratio in the atmospheres of Uranus and Neptune from Herschel-PACS observations. Astron. Astrophys. 551, A126 (2013).
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