Thermal emission from WASP-33b, the hottest known planet

Monthly Notices of the Royal Astronomical Society

Volumn 416, Issue 3, 2011, Pages 2096-2101

  Smith, A M S ^a   Anderson, D R ^a   Skillen, I ^b   Cameron, A Collier ^c   Smalley, B ^a  

^a KEELE UNIVERSITY   (United Kingdom)

^b ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

^c UNIVERSITY OF ST ANDREWS   (United Kingdom)

Author keywords

Infrared: planetary systems; Planetary systems; Stars: individual: WASP 33; Stars: oscillations; Stars: variables: Scuti

Indexed keywords

HOST-STARS; INFRARED: PLANETARY SYSTEMS; PLANETARY SYSTEM; RE-RADIATION; STAR OSCILLATIONS; STAR: INDIVIDUAL: WASP-33; STAR: VARIABLE: Δ SCUTI; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: VARIABLES; Δ SCUTI;

STARS;

EID: 80052621730     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.19187.x     Document Type: Article

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