An Enigmatic Pointlike Feature within the HD 169142 Transitional Disk
arXiv:1408.0794 · doi:10.1088/2041-8205/792/1/L22
Abstract
We report the detection of a faint pointlike feature possibly related to ongoing planet-formation in the disk of the transition disk star HD 169142. The pointlike feature has a mag(L)6.4, at a separation of 0.11" and PA0. Given its lack of an H or K counterpart despite its relative brightness, this candidate cannot be explained by purely photospheric emission and must be a disk feature heated by an as yet unknown source. Its extremely red colors make it highly unlikely to be a background object, but future multi-wavelength followup is necessary for confirmation and characterization of this feature.
Accepted to ApJ Letters, see also Reggiani et al. 2014
References in corpus (4)
- Direct Imaging of Multiple Planets Orbiting the Star HR 8799
- Demographics of Transition Objects
- Discovery of a Companion Candidate in the HD169142 Transition Disk and the Possibility of Multiple Planet Formation
- Magellan Adaptive Optics first-light observations of the exoplanet Pic b. I. Direct imaging in the far-red optical with MagAO+VisAO and in the near-IR with NICI
Cited by in corpus (10)
- Accreting Circumplanetary Disks: Observational Signatures
- Discovery of a Companion Candidate in the HD169142 Transition Disk and the Possibility of Multiple Planet Formation
- Recovery of the Candidate Protoplanet HD 100546 b with Gemini/NICI and Detection of Additional (Planet-Induced?) Disk Structure at Small Separations
- Five steps in the evolution from protoplanetary to debris disk
- Variability of Disk Emission in Pre-Main Sequence and Related Stars. III. Exploring Structural Changes in the Pre-transitional Disk in HD 169142
- Spectral Energy Distributions of Accreting Protoplanets
- Searching for Planets in Holey Debris Disks with the Apodizing Phase Plate
- The Transitional Disk around IRAS 04125+2902
- Herbig AeBe stars: Multiplicity and consequences
- High-contrast imaging constraints on gas giant planet formation - The Herbig Ae/Be star opportunity