Analysis of new high-precision transit light curves of WASP-10 b: Starspot occultations, small planetary radius, and high metallicity

Astronomy and Astrophysics

Volumn 535, Issue , 2011, Pages

  Maciejewski, G ^a,b   Raetz, St ^b   Nettelmann, N ^c   Seeliger, M ^b   Adam, C ^b   Nowak, G ^a   Neuhauser R ^b  

^a NICOLAUS COPERNICUS UNIVERSITY   (Poland)

^b Astrophysikalisches Institut und Universitats Sternwarte Jena   (Germany)

^c UNIVERSITY OF ROSTOCK   (Germany)

Author keywords

planets and satellites: individual: WASP 10 b; stars: individual: WASP 10; Starspots

Indexed keywords

BEST-FIT MODELS; DARK SPOTS; EARTH MASS; ERROR ESTIMATES; EXOPLANET; HEAVY ELEMENTS; HIGH-PRECISION; HOST-STARS; INTERIOR STRUCTURE; INTERNAL STRUCTURE; JUPITERS; LIGHT CURVES; LITERATURE DATA; MEAN DENSITY; METALLICITIES; MONTE CARLO SIMULATION; ORBITAL MOTIONS; PERIODIC MODULATION; PERIODIC VARIATION; PHYSICAL PARAMETERS; PLANETARY SYSTEM; PLANETS AND SATELLITES: INDIVIDUAL: WASP-10 B; ROCK CORE; ROTATIONAL MODULATION; STARS: INDIVIDUAL; STARSPOTS; STELLAR DISKS; TRANSIT TIMING; TWO-LAYER STRUCTURES;

ASTROPHYSICS; CHEMICAL ELEMENTS; COMPUTER SIMULATION; MONTE CARLO METHODS; STARS;

EARTH (PLANET);

EID: 80054912402     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117127     Document Type: Article

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