How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits
about
Defining and cataloging exoplanets: the exoplanet.eu databaseHabitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD 40307Benchmarking the power of amateur observatories for TTV exoplanets detectionThe properties of planets around giant starsDisentangling 2:1 resonant radial velocity orbits from eccentric ones and a case study for HD 27894Improved signal detection algorithms for unevenly sampled data. Six signals in the radial velocity data for GJ876Stable habitable zones of single Jovian planet systemsThe SOPHIE search for northern extrasolar planets. X. Detection and characterization of giant planets by the dozenRadial velocity data analysis with compressed sensing techniquesDetectability of quasi-circular co-orbital planets. Application to the radial velocity techniqueStellar wobble caused by a nearby binary system: eccentric and inclined orbits
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How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits
description
article publié dans la revue scientifique Astrophysical Journal
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im Dezember 2009 veröffentlichter wissenschaftlicher Artikel
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scientific article published in the Astrophysical Journal
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wetenschappelijk artikel
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наукова стаття, опублікована в грудні 2009
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name
HOW ECCENTRIC ORBITAL SOLUTIONS CAN HIDE PLANETARY SYSTEMS IN 2:1 RESONANT ORBITS
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How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits
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type
label
HOW ECCENTRIC ORBITAL SOLUTIONS CAN HIDE PLANETARY SYSTEMS IN 2:1 RESONANT ORBITS
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How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits
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prefLabel
HOW ECCENTRIC ORBITAL SOLUTIONS CAN HIDE PLANETARY SYSTEMS IN 2:1 RESONANT ORBITS
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How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits
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P1476
How eccentric orbital solutions can hide planetary systems in 2:1 resonant orbits
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John E. Chambers
Mercedes López-Morales
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10.1088/0004-637X/709/1/168
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P577
2009-12-29T00:00:00Z
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P819
2010ApJ...709..168A