Coronagraphic observations of Fomalhaut at solar system scales
arXiv:1212.1459 · doi:10.1088/0004-637X/764/1/7
Abstract
We report on a search for low mass companions within 10 AU of the star Fomalhaut, using narrow band observations at 4.05 microns obtained with the Apodizing Phase Plate (APP) coronagraph on the VLT/NaCo. Our observations place a model dependent upper mass limit of 12-20 Jupiter masses from 4 to 10 AU, covering the semi-major axis search space between interferometric imaging measurements and other direct imaging non-detections. These observations rule out models where the large semi-major axis for the putative candidate companion Fomalhaut b is explained by dynamical scattering from a more massive companion in the inner stellar system, where such giant planets are thought to form.
18 pages, 4 figures, to be published in ApJ
References in corpus (10)
- Direct Imaging of Multiple Planets Orbiting the Star HR 8799
- Rapid growth of gas-giant cores by pebble accretion
- Optical Images of an Exosolar Planet 25 Light Years from Earth
- On the Age and Binarity of Fomalhaut
- The International Deep Planet Survey I. The frequency of wide-orbit massive planets around A-stars
- First Light LBT AO Images of HR 8799 bcde at 1.65 and 3.3 Microns: New Discrepancies between Young Planets and Old Brown Dwarfs
- Herschel images of Fomalhaut. An extrasolar Kuiper Belt at the height of its dynamical activity
- Spitzer/IRAC Limits to Planetary Companions of Fomalhaut and epsilon Eridani
- Thermal Infrared Constraint to a Planetary Companion of Vega with the MMT Adaptive Optics System
- Searching for young Jupiter analogs around AP Col: L-band high-contrast imaging of the closest pre-main sequence star
Cited by in corpus (27)
- Fundamental limitations of high contrast imaging set by small sample statistics
- Imaging Extrasolar Giant Planets
- Combining high-dispersion spectroscopy (HDS) with high contrast imaging (HCI): Probing rocky planets around our nearest neighbors
- A young protoplanet candidate embedded in the circumstellar disk of HD100546
- Constraining the initial entropy of directly-detected exoplanets
- STIS Coronagraphic Imaging of Fomalhaut: Main Belt Structure and the Orbit of Fomalhaut b
- Dynamical evolution of an eccentric planet and a less massive debris disc
- The SEEDS Direct Imaging Survey for Planets and Scattered Dust Emission in Debris Disk Systems
- L'-band AGPM vector vortex coronagraph's first light on VLT/NACO: Discovery of a late-type companion at two beamwidths from an F0V star
- An independent determination of Fomalhaut b's orbit and the dynamical effects on the outer dust belt
- Laboratory demonstration of a mid-infrared AGPM vector vortex coronagraph
- On-sky performance analysis of the vector Apodizing Phase Plate coronagraph on MagAO/Clio2
- High-contrast Imaging with Spitzer: Deep Observations of Vega, Fomalhaut, and epsilon Eridani
- Spatially resolved imaging of the inner Fomalhaut disk using JWST/MIRI
- Spectroscopic Signatures of Extra-Tidal Stars Around the Globular Clusters NGC 6656 (M22), NGC 3201 and NGC 1851 from RAVE
- Optimized Principal Component Analysis on Coronagraphic Images of the Fomalhaut System
- Discovery of the Fomalhaut C debris disc
- Searching for Planets in Holey Debris Disks with the Apodizing Phase Plate
- Search for cool giant exoplanets around young and nearby stars - VLT/NaCo near-infrared phase-coronagraphic and differential imaging
- Fomalhaut b could be massive and sculpting the narrow, eccentric debris disc, if in mean-motion resonance with it
- Discovery of a Low-Mass Companion to the F7V star HD 984
- Searching for gas giant planets on Solar System scales - A NACO/APP L'-band survey of A- and F-type Main Sequence stars
- The companion candidate near Fomalhaut - a background neutron star?
- A Deep Keck/NIRC2 Search for Thermal Emission from Planetary Companions Orbiting Fomalhaut
- Imaged sub-stellar companions: not as eccentric as they appear? The effect of an unseen inner mass on derived orbits
- ALMA imaging of the M-dwarf Fomalhaut C's debris disc
- Sparse aperture masking at the VLT II. Detection limits for the eight debris disks stars Pic, AU Mic, 49 Cet, Tel, Fomalhaut, g Lup, HD181327 and HR8799