Mapping the Planetary Wake in HD 163296 with Kinematics
arXiv:2111.07416 · doi:10.3847/2041-8213/ac64a7
Abstract
We map the planetary wake associated with the embedded protoplanet creating the CO kink in the disk of HD~163296. We show that the wake can be traced by a series of correlated perturbations in the peak velocity map. The sign change of the perturbations across the disk major axis confirm that the wake induces predominantly radial motion, as predicted by models of planet-disk interaction. These results provide the first direct confirmation of planet wakes generated by Lindblad resonances. Mapping the wake provides a constraint on the disk aspect ratio, which is required to measure the mass of the planet.
10 Pages, 6 figures. Accepted in ApJL
References in corpus (9)
- SPLASH: An interactive visualisation tool for Smoothed Particle Hydrodynamics simulations
- Monte Carlo radiative transfer in protoplanetary disks
- Molecules with ALMA at Planet-forming Scales (MAPS) I: Program Overview and Highlights
- Direct mapping of the temperature and velocity gradients in discs. Imaging the vertical CO snow line around IM Lupi
- Molecules with ALMA at Planet-forming Scales (MAPS) IV: Emission Surfaces and Vertical Distribution of Molecules
- A new planet candidate detected in a dust gap of the disc around HD 163296 through localised kinematic signatures. An observational validation of the Discminer
- Spiral arms in thermally stratified protoplanetary discs
- The theory of kinks -- I. A semi-analytic model of velocity perturbations due to planet-disc interaction
- Constraining Protoplanetary Disk Accretion and Young Planets Using ALMA Kinematic Observations
Cited by in corpus (21)
- The Disc Miner II: Revealing Gas substructures and Kinematic signatures from Planet-disc interaction through line profile analysis
- Kinematics and brightness temperatures of transition discs -- A survey of gas substructures as seen with ALMA
- Mapping the Complex Kinematic Substructure in the TW Hya Disk
- Mapping Protoplanetary Disk Vertical Structure with CO Isotopologue Line Emission
- Rotation curves in protoplanetary disks with thermal stratification
- exoALMA III: Line-intensity Modeling and System Property Extraction from Protoplanetary Disks
- A kinematically detected planet candidate in a transition disk
- The Origin of the Doppler-flip in HD 100546: a large scale spiral arm generated by an inner binary companion
- Kinematic evidence for an embedded planet in the IM Lupi disc
- A localized kinematic structure detected in atomic carbon emission spatially coincident with a proposed protoplanet in the HD 163296 disk
- Kinematic and thermal signatures of the directly imaged protoplanet candidate around Elias 2-24
- DBNets: A publicly available deep learning tool to measure the masses of young planets in dusty protoplanetary discs
- Testing velocity kinks as a planet-detection method: Do velocity kinks in surface gas emission trace planetary spiral wakes in the midplane continuum?
- exoALMA. VIII. Probabilistic Moment Maps and Data Products using Non-parametric Linear Models
- Observational Signatures of Circumbinary Discs I: Kinematics
- Kinematics signature of a giant planet in the disk of AS 209
- Circumplanetary Disk Candidate in the Disk of HD 163296 Traced by Localized Emission from Simple Organics
- Continuing to Hide Signatures of Gravitational Instability in Protoplanetary Discs with Planets
- exoALMA XX: Tomographic Detection of Embedded Planets in Protoplanetary Disks
- -mapping of planet-induced density wave damping in protoplanetary discs
- CO Line Emission Surfaces and Vertical Structure in Mid-Inclination Protoplanetary Disks