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Possible Solutions to the Radius Anomalies of Transiting Giant Planets

Possible Solutions to the Radius Anomalies of Transiting Giant Planets

http://www.wikidata.org/entity/Q56031861

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The EChO science case Photometric and spectroscopic detection of the primary transit of the 111-day-period planet HD 80 606 b Structure of exoplanets.Improved parameters for the transiting hot Jupiters WASP-4b and WASP-5b Discovery and characterization of WASP-6b, an inflated sub-Jupiter mass planet transiting a solar-type star High-precision transit observations of the exoplanet WASP-13b with the RISE instrument WASP-54b, WASP-56b, and WASP-57b: Three new sub-Jupiter mass planets from SuperWASP Transiting exoplanets from the CoRoT space mission. I. CoRoT-Exo-1b: a low-density short-period planet around a G0V star Rayleigh scattering by H2 in the extrasolar planet HD 209458b SOPHIE velocimetry ofKeplertransit candidates Towards closing the window on strongly interacting dark matter: Far-reaching constraints from Earth’s heat flow Transiting exoplanets from the CoRoT space mission. V. CoRoT-Exo-4b: stellar and planetary parameters WASP-121 b: a hot Jupiter close to tidal disruption transiting an active F star HAT-P-38b: A Saturn-Mass Planet Transiting a Late G Star Physical properties and radius variations in the HAT-P-5 planetary system from simultaneous four-colour photometry WASP-42 b and WASP-49 b: two new transiting sub-Jupiters Thermal emission at 4.5 and 8 μm of WASP-17b, an extremely large planet in a slightly eccentric orbit WASP-31b: a low-density planet transiting a metal-poor, late-F-type dwarf star WASP-39b: a highly inflated Saturn-mass planet orbiting a late G-type star New and updated stellar parameters for 90 transit hosts Understanding exoplanet formation, structure and evolution in 2010 Uncertainties in tidal theory: Implications for bloated hot Jupiters The Young Exoplanet Transit Initiative (YETI)From dense hot Jupiter to low-density Neptune: The discovery of WASP-127b, WASP-136b, and WASP-138b WASP-113b and WASP-114b, two inflated hot Jupiters with contrasting densities SOPHIE velocimetry of Kepler transit candidates. XVII. The physical properties of giant exoplanets within 400 days of period Discovery of WASP-65b and WASP-75b: Two hot Jupiters without highly inflated radii New transiting exoplanets from the SuperWASP-North survey Tidal dissipation in multi-planet systems and constraints on orbit fitting A possible correlation between planetary radius and orbital period for small planets Physical properties of the WASP-44 planetary system from simultaneous multi-colour photometry

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Possible Solutions to the Radius Anomalies of Transiting Giant Planets

http://www.wikidata.org/entity/Q56031861

description

article publié dans la revue scientifique Astrophysical Journal

@fr

im Mai 2007 veröffentlichter wissenschaftlicher Artikel

@de

scientific article published in the Astrophysical Journal

@en

wetenschappelijk artikel

@nl

наукова стаття, опублікована в травні 2007

@uk

name

Possible Solutions to the Radius Anomalies of Transiting Giant Planets

@en

Possible Solutions to the Radius Anomalies of Transiting Giant Planets

@nl

type

label

Possible Solutions to the Radius Anomalies of Transiting Giant Planets

@en

Possible Solutions to the Radius Anomalies of Transiting Giant Planets

@nl

prefLabel

Possible Solutions to the Radius Anomalies of Transiting Giant Planets

@en

Possible Solutions to the Radius Anomalies of Transiting Giant Planets

@nl

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Letters of the Astrophysical Journal

The Astrophysical Journal

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Possible Solutions to the Radius Anomalies of Transiting Giant Planets

@en

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A. Burrows

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I. Hubeny

http://www.w3.org/2001/XMLSchema#string

J. Budaj

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W. B. Hubbard

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502–514

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scholarly article

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10.1086/514326

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P433

1

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661

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2007-05-20T00:00:00Z

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1805656

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astro-ph/0612703

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2007ApJ...661..502B

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