Improving Planet Detection with Disk Modeling: Keck/NIRC2 Imaging of the HD 34282 Single-armed Protoplanetary Disk

Formed in protoplanetary disks around young stars, giant planets can leave observational features such as spirals and gaps in their natal disks through planet–disk interactions. Although such features can indicate the existence of giant planets, protoplanetary disk signals can overwhelm the innate l...

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Veröffentlicht in:	Astrophysical journal. Letters 2022-01, Vol.924 (1), p.L4
Hauptverfasser:	Quiroz, Juan, Wallack, Nicole L., Ren, Bin, Dong, Ruobing, Xuan, Jerry W., Mawet, Dimitri, Millar-Blanchaer, Maxwell A., Ruane, Garreth
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Coronagraphic imaging Coronagraphs Detection limits Jupiter Luminosity Modelling Planet detection Planet formation Planetary system formation Planets Protoplanetary disks Space telescopes Spirals
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