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Gravitoviscous protoplanetary disks with a dust component
- Source :
- Astron. Astrophys., Astronomy and Astrophysics
- Publication Year :
- 2020
- Publisher :
- EDP Sciences, 2020.
-
Abstract
- We study the dynamics and growth of dust particles in circumstellar disks of different masses that are prone to gravitational instability during the critical first Myr of their evolution. The dust component is made up of two different components: micron-sized dust and grown dust of evolving size. For the dust component, we considered the dust coagulation, fragmentation, momentum exchange with the gas, and dust self-gravity. We found that the micron-sized dust particles grow rapidly in the circumstellar disk, reaching a few cm in size in the inner 100 au of the disk during less than 100 kyr after the disk formation, provided that fragmentation velocity is $30\rm~ms^{-1}$. Due to the accretion of micron dust particles from the surrounding envelope, which serves as a micron dust reservoir, the approximately cm-sized dust particles continue to be present in the disk for more than 900 kyr after the disk formation and maintain a dust-to-gas ratio close to 0.01. We show that a strong correlation exists between the gas and pebble fluxes in the disk. We find that radial surface density distribution of pebbles in the disk shows power-law distribution with an index similar to that of the Minimum-mass solar nebula (MMSN) regardless the disk mass. We also show that the gas surface density in our models agrees well with measurements of dust in protoplanetary disks of AS 209, HD 163296, and DoAr 25 systems. Pebbles are formed during the very early stages of protoplanetary disk evolution. They play a crucial role in the planet formation process. Our disc simulations reveal the early onset ($<br />13 pages, 10 figures
- Subjects :
- Mass flux
Planetesimal
010504 meteorology & atmospheric sciences
FOS: Physical sciences
DUST
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics
GASES
Protoplanetary disk
NUMERICAL HYDRODYNAMICS
01 natural sciences
HYDRODYNAMICS
Planet
FORMATION [STARS]
0103 physical sciences
Astrophysics::Solar and Stellar Astrophysics
DENSITY OF GASES
Pebble
010303 astronomy & astrophysics
SOLAR POWER GENERATION
Astrophysics::Galaxy Astrophysics
HYDRODYNAMICS EQUATION
0105 earth and related environmental sciences
Earth and Planetary Astrophysics (astro-ph.EP)
Physics
POWER LAW DISTRIBUTION
GRAVITATION
Astronomy and Astrophysics
Accretion (astrophysics)
FORMATION AND EVOLUTIONS
13. Climate action
Space and Planetary Science
GRAVITATIONAL INSTABILITY
Streaming instability
Astrophysics::Earth and Planetary Astrophysics
GLOBAL NUMERICAL SIMULATIONS
Formation and evolution of the Solar System
SURFACE DENSITY DISTRIBUTION
PROTOPLANETARY DISKS
STARS
Astrophysics - Earth and Planetary Astrophysics
Subjects
Details
- ISSN :
- 14320746 and 00046361
- Volume :
- 637
- Database :
- OpenAIRE
- Journal :
- Astronomy & Astrophysics
- Accession number :
- edsair.doi.dedup.....1bd845b6ed61880620dda5bba759d373