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pro vyhledávání: '"Husnoo, Nawal"'
Autor:
Husnoo, Nawal, Pont, Frederic, Hebrard, Guillaume, Simpson, Elaine, Mazeh, Tsevi, Bouchy, Francois, Moutou, Claire, Arnold, Luc, Boisse, Isabelle, Diaz, Rodrigo, Eggenberger, Anne, Shporer, Avi
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2011, 413 (4), pp.2500--2508. ⟨10.1111/j.1365-2966.2011.18322.x⟩
Monthly Notices of the Royal Astronomical Society, 2011, 413 (4), pp.2500--2508. ⟨10.1111/j.1365-2966.2011.18322.x⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2011, 413 (4), pp.2500--2508. ⟨10.1111/j.1365-2966.2011.18322.x⟩
Monthly Notices of the Royal Astronomical Society, 2011, 413 (4), pp.2500--2508. ⟨10.1111/j.1365-2966.2011.18322.x⟩
As part of the long-term radial velocity monitoring of known transiting planets -- designed to measure orbital eccentricities, spin-orbit alignments and further planetary companions -- we have acquired radial velocity data for the two transiting syst
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::35ea0d92f06d0d7f3640fe7c246433a1
https://hal.archives-ouvertes.fr/hal-01438031
https://hal.archives-ouvertes.fr/hal-01438031
The two dominant features in the distribution of orbital parameters for close-in exoplanets are the prevalence of circular orbits for very short periods, and the observation that planets on closer orbits tend to be heavier. The first feature is inter
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2406ffab37bb06161e63a6737fc9c4ae
http://arxiv.org/abs/1103.2081
http://arxiv.org/abs/1103.2081