Infrared non-detection of Fomalhaut b: implications for the planet interpretation
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Formation of sharp eccentric rings in debris disks with gas but without planets.Direct imaging of exoplanets.Herschelimages of FomalhautHigh-contrast imaging withSpitzer: deep observations of Vega, Fomalhaut, andϵEridaniRapid growth of gas-giant cores by pebble accretionAn interferometric study of the Fomalhaut inner debris disk. III. Detailed models of the exozodiacal disk and its originThe International Deep Planet SurveyA test of the neutron star hypothesis for Fomalhaut b
P2860
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P2860
Infrared non-detection of Fomalhaut b: implications for the planet interpretation
description
article publié dans la revue scientifique Astrophysical Journal
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im Februar 2012 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 лютому 2012
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name
INFRARED NON-DETECTION OF FOMALHAUT b: IMPLICATIONS FOR THE PLANET INTERPRETATION
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Infrared non-detection of Fomalhaut b: implications for the planet interpretation
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type
label
INFRARED NON-DETECTION OF FOMALHAUT b: IMPLICATIONS FOR THE PLANET INTERPRETATION
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Infrared non-detection of Fomalhaut b: implications for the planet interpretation
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prefLabel
INFRARED NON-DETECTION OF FOMALHAUT b: IMPLICATIONS FOR THE PLANET INTERPRETATION
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Infrared non-detection of Fomalhaut b: implications for the planet interpretation
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P2093
P356
P1476
Infrared non-detection of Fomalhaut b: implications for the planet interpretation
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P2093
David S. Spiegel
John R. Bent
Joseph C. Carson
Markus Janson
Palmer Wong
P356
10.1088/0004-637X/747/2/116
P407
P577
2012-02-23T00:00:00Z
P818
P819
2012ApJ...747..116J