3.6 AND 4.5 μm PHASE CURVES OF THE HIGHLY IRRADIATED ECCENTRIC HOT JUPITER WASP-14b

Autor: Wong, I, Knutson, HA, Lewis, NK, Kataria, T, Burrows, A, Fortney, JJ, Schwartz, J, Agol, E, Cowan, NB, Deming, D, Désert, JM, Fulton, BJ, Howard, AW, Langton, J, Laughlin, G, Showman, AP, Todorov, K

Publikováno v: The Astrophysical Journal, vol 811, iss 2
Astrophysical Journal, vol 811, iss 2
Wong, I; Knutson, HA; Lewis, NK; Kataria, T; Burrows, A; Fortney, JJ; et al.(2015). 3.6 and 4.5 μm PHASE CURVES of the HIGHLY IRRADIATED ECCENTRIC HOT JUPITER WASP-14b. Astrophysical Journal, 811(2). doi: 10.1088/0004-637X/811/2/122. UC Santa Cruz: Retrieved from: http://www.escholarship.org/uc/item/35s7v6mg

© 2015. The American Astronomical Society. All rights reserved.. We present full-orbit phase curve observations of the eccentric (e ∼ 0.08) transiting hot Jupiter WASP-14b obtained in the 3.6 and 4.5 μm bands using the Spitzer Space Telescope. We

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::75a0edf8478483ce32dd4bd19b358653
https://escholarship.org/uc/item/35s7v6mg

Zones, spots, and planetary-scale waves beating in brown dwarf atmospheres.

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