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Modeling Dust Emission of HL Tau Disk Based on Planet-Disk Interactions

Journal Article · · The Astrophysical Journal (Online)
 [1];  [2];  [3];  [2];  [4]
  1. Chinese Academy of Sciences (CAS), Nanjing (China). Purple Mountain Observatory. Key Lab. of Planetary Sciences; Los Alamos National Lab. (LANL), Los Alamos, NM (United States). Theoretical Division
  2. Los Alamos National Lab. (LANL), Los Alamos, NM (United States). Theoretical Division
  3. Rice Univ., Houston, TX (United States)
  4. Chinese Academy of Sciences (CAS), Nanjing (China). Purple Mountain Observatory. Key Lab. of Planetary Sciences
+ Show Author Affiliations
In this paper, we use extensive global two-dimensional hydrodynamic disk gas+dust simulations with embedded planets, coupled with three-dimensional radiative transfer calculations, to model the dust ring and gap structures in the HL Tau protoplanetary disk observed with the Atacama Large Millimeter/Submillimeter Array (ALMA). We include the self-gravity of disk gas and dust components and make reasonable choices of disk parameters, assuming an already settled dust distribution and no planet migration. We can obtain quite adequate fits to the observed dust emission using three planets with masses of 0.35, 0.17, and 0.26 MJup at 13.1, 33.0, and 68.6 AU, respectively. Finally, implications for the planet formation as well as the limitations of this scenario are discussed.
Research Organization:
Chinese Academy of Sciences (CAS), Nanjing (China); Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
Chinese Academy of Sciences (China); National Aeronautics and Space Administration (NASA) (United States); National Natural Science Foundation (China); National Science Foundation (NSF) (United States); Natural Science Foundation of Jiangsu Province (China); USDOE Laboratory Directed Research and Development (LDRD) Program
Contributing Organization:
Rice Univ., Houston, TX (United States)
Grant/Contract Number:
AC52-06NA25396
OSTI ID:
1335605
Alternate ID(s):
OSTI ID: 22521571
Report Number(s):
LA-UR--15-28170
Journal Information:
The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 1 Vol. 818; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English

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HL Tau Disk in HCO + (3–2) and (1–0) with ALMA: Gas Density, Temperature, Gap, and One-arm Spiral journal July 2019
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The Radial Distribution of Dust Particles in the HL Tau Disk from ALMA and VLA Observations journal September 2019
Including Dust Coagulation in Hydrodynamic Models of Protoplanetary Disks: Dust Evolution in the Vicinity of a Jupiter-mass Planet journal November 2019
On the Dust Signatures Induced by Eccentric Super-Earths in Protoplanetary Disks journal November 2019
Exploring the Grain Properties in the Disk of HL Tau with an Evolutionary Model journal December 2019
Diverse Protoplanetary Disk Morphology Produced by a Jupiter-mass Planet journal September 2018
The Disk Substructures at High Angular Resolution Project (DSHARP). VII. The Planet–Disk Interactions Interpretation journal December 2018
The Disk Substructures at High Angular Resolution Project (DSHARP). IX. A High-definition Study of the HD 163296 Planet-forming Disk journal December 2018
The Observability of Vortex-driven Spiral Arms in Protoplanetary Disks: Basic Spiral Properties journal September 2019
Catastrophic Events in Protoplanetary Disks and Their Observational Manifestations journal December 2019
Signatures of Young Planets in the Continuum Emission From Protostellar Disks preprint January 2016
What is the Mass of a Gap-Opening Planet? text January 2016
Investigating the early evolution of planetary systems with ALMA and the Next Generation Very Large Array text January 2018
CO and dust properties in the TW Hya disk from high-resolution ALMA observations text January 2018
Rings and gaps in the disc around Elias 24 revealed by ALMA text January 2018
Is the spiral morphology of the Elias 2-27 circumstellar disc due to gravitational instability? text January 2018
Applying a Particle-only Model to the HL Tau Disk text January 2018
ALMA observations of polarization from dust scattering in the IM Lup protoplanetary disk text January 2018
Diverse protoplanetary disk morphology produced by a Jupiter-mass planet text January 2018
The Ring Structure in the MWC 480 Disk Revealed by ALMA text January 2018
The Disk Substructures at High Angular Resolution Project (DSHARP): VII. The Planet-Disk Interactions Interpretation text January 2018
The Disk Substructures at High Angular Resolution Project (DSHARP) - IX. A high definition study of the HD 163296 planet forming disk text January 2018
Pebble accretion in class 0/I YSOs as a possible pathway for early planet formation text January 2019
Dust continuum emission and the upper limit fluxes of sub-millimeter water lines of the protoplanetary disk around HD 163296 observed by ALMA text January 2019
A dust and gas cavity in the disc around CQ Tau revealed by ALMA text January 2019
New constraints on the dust and gas distribution in the LkCa 15 disk from ALMA text January 2019
The Observability Of Vortex-Driven Spiral Arms In Protoplanetary Disk: Basic Spiral Properties text January 2019
On the Dust Signatures Induced by Eccentric Super-Earths in Protoplanetary Disks text January 2019

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Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
astronomy and astrophysics
planet–disk interactions
protoplanetary disks
submillimeter: planetary systems
techniques: interferometric