One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c
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Understanding stellar activity-induced radial velocity jitter using simultaneous K2 photometry and HARPS RV measurementsPhotodynamical mass determination of the multiplanetary system K2-19Mass determination of K2-19b and K2-19c from radial velocities and transit timing variationsThe Way ForwardSingle transit candidates from K2: detection and period estimationThe K2-ESPRINT project. VI. K2-105 b, a hot Neptune around a metal-rich G-dwarf
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One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c
description
article publié dans la revue scientifique Astronomy and Astrophysics
@fr
im Oktober 2015 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in Astronomy and Astrophysics
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wetenschappelijk artikel
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наукова стаття, опублікована в жовтні 2015
@uk
name
One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c
@en
One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c
@nl
type
label
One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c
@en
One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c
@nl
prefLabel
One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c
@en
One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c
@nl
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One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c
@en
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Amanda P. Doyle
Arvind Rajpurohit
Bastien Courcol
David J. A. Brown
David J. Armstrong
Don L. Pollacco
Giovanni Bruno
Hugh P. Osborn
Isabelle Boisse
James Kirk
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10.1051/0004-6361/201526008
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P50
P577
2015-10-01T00:00:00Z
P818
1503.00692
P819
2015A&A...582A..33A