A possible tilted orbit of the super-Neptune HAT-P-11b

Publications of the Astronomical Society of Japan

Volumn 63, Issue SPEC. ISSUE 2, 2011, Pages

  Hirano, Teruyuki ^a,b   Narita, Norio ^c   Shporer, Avi ^d,e   Sato, Bun'ei ^f   Aoki, Wako ^c   Tamura, Motohide ^c  

^a UNIVERSITY OF TOKYO   (Japan)

^b MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^c NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e LAS CUMBRES OBSERVATORY GLOBAL TELESCOPE NETWORK   (United States)

^f TOKYO INSTITUTE OF TECHNOLOGY   (Japan)

Author keywords

Stars: planetary systems: individual (HAT P 11); Stars: rotation; Techniques: photometric; Techniques: radial velocities; Techniques: spectroscopic

Indexed keywords

ALIGNMENT; EARTH (PLANET); ORBITS; PHOTOMETRY; PLANETS; TELESCOPES;

EXO-PLANETS; NEPTUNE; RADIAL VELOCITY MEASUREMENTS; SPIN ORBITS; STAR: PLANETARY SYSTEM: INDIVIDUAL (HAT-P-11); STARS: PLANETARY SYSTEM; STARS: ROTATION; TECHNIQUES: PHOTOMETRIC; TECHNIQUES: RADIAL VELOCITIES; TECHNIQUES: SPECTROSCOPIC;

STARS;

EID: 79953328290     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/63.sp2.S531     Document Type: Article

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