12 Feb 2011: Hashimoto et al. (2011) do not confirm the point source suspected by Oppenheimer et al. (2008). Nevertheless, various gaps and warps in the disk lead to suspect the presence of planets (Hashimoto et al. 2011). 22 Nov 2008: Oppenheimer et al (2008) report this object as "a low significances detection".
The likelihood of not detecting cavity-carving companions in transition discs -- A statistical approach
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, accepted
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Predictions of Dust Continuum Emission from a Potential Circumplanetary Disk: A Case Study of the Planet Candidate AB Aurigae b
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Mapping the merging zone of late infall in the AB Aur planet-forming system
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VLT/MUSE Hα and Hβ observations of the AB Aur planetary system
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Gap-opening Planets Make Dust Rings Wider
BI J., LIN M.-K. & DONG R.
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AB Aur, a Rosetta stone for studies of planet formation (III): continuum observations at 2 and 7 mm
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arxiv
UV-Optical Emission of AB Aur b is Consistent with Scattered Stellar Light
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Images of embedded Jovian planet formation at a wide separation around AB Aurigae
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Nature Astronomy
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AB Aurigae: Possible evidence of planet formation through the gravitational instability
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AB Aur, a Rosetta stone for studies of planet formation. I. Chemical study of a planet-forming disk
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, 642
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The Separation and Hα Contrasts of Massive Accreting Planets in the Gaps of Transitional Disks: Predicted Hα Protoplanet Yields for Adaptive Optics Surveys
Radiative Transfer Models of a Possible Planet in the AB Aurigae Disk
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High-Contrast Observations in Optical and Infrared Astronomy
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