Article (Scientific journals)
Thermal emission at 3.6-8 micron from WASP-19b: a hot Jupiter without a stratosphere orbiting an active star
Anderson, D. R.; Smith, A. M. S.; Madhusudhan, N. et al.
2013In Monthly Notices of the Royal Astronomical Society, 430 (4), p. 3422-3431
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Keywords :
Astrophysics - Earth and Planetary Astrophysics
Abstract :
[en] We report detection of thermal emission from the exoplanet WASP-19b at 3.6, 4.5, 5.8 and 8.0 μm. We used the InfraRed Array Camera on the Spitzer Space Telescope to observe two occultations of WASP-19b by its host star. We combine our new detections with previous measurements of WASP-19b's emission at 1.6 and 2.09 μm to construct a spectral energy distribution of the planet's dayside atmosphere. By comparing this with model-atmosphere spectra, we find that the dayside atmosphere of WASP-19b lacks a strong temperature inversion. As WASP-19 is an active star (log R'HK = -4.50 ± 0.03), this finding supports the hypothesis of Knutson, Howard and Isaacson that inversions are suppressed in hot Jupiters orbiting active stars. The available data are unable to differentiate between a carbon-rich and an oxygen-rich atmosphere.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Anderson, D. R.
Smith, A. M. S.
Madhusudhan, N.
Wheatley, P. J.
Collier Cameron, A.
Hellier, C.
Campo, C.
Gillon, Michaël  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique et traitement de l'image
Harrington, J.
Maxted, P. F. L.
Pollacco, D.
Queloz, D.
Smalley, B.
Triaud, A H M J
West, R. G.
More authors (5 more) Less
Language :
English
Title :
Thermal emission at 3.6-8 micron from WASP-19b: a hot Jupiter without a stratosphere orbiting an active star
Publication date :
01 April 2013
Journal title :
Monthly Notices of the Royal Astronomical Society
ISSN :
0035-8711
eISSN :
1365-2966
Publisher :
Blackwell Publishing, Oxford, United Kingdom
Volume :
430
Issue :
4
Pages :
3422-3431
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
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