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1. Full Text Observational signatures of planets in protoplanetary disks. I. Gaps opened by single and multiple young planets in disks
by Dong, Ruobing and Zhu, Zhaohuan and Whitney, Barbara
Astrophysical Journal, ISSN 0004-637X, 08/2015, Volume 809, Issue 1, pp. 93 - 18
It has been suggested that the gaps and cavities recently discovered in transitional disks are opened by planets. To explore this scenario, we combine... 
stars: pre-main sequence | planet-disk interactions | protoplanetary disks | stars: variables: T Tauri, Herbig Ae/Be | planets and satellites: formation | circumstellar matter | LOW-MASS PLANETS | GIANT PLANET | PROTOSTELLAR ENVELOPES | SPITZER IRS | DUST FILTRATION | ASTRONOMY & ASTROPHYSICS | CIRCUMSTELLAR DISK | 2-DIMENSIONAL RADIATIVE-TRANSFER | IMAGING POLARIMETRY | TRANSITIONAL DISK | PRETRANSITIONAL DISKS | Planets | Wavelengths | Computer simulation | Planet formation | Radiative transfer | Signatures | Accretion disks | Three dimensional | Physics - Earth and Planetary Astrophysics
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2. Full Text Gaps, rings, and non-Axisymmetric structures in protoplanetary disks From simulations to ALMA observations
by Flock, M and Ruge, J.P and Dzyurkevich, N and Henning, Th and Klahr, H and Wolf, S
Astronomy and Astrophysics, ISSN 0004-6361, 2015, Volume 574, p. A68
Aims. Recent observations by the Atacama Large Millimeter/submillimeter Array (ALMA) of disks around young stars revealed distinct asymmetries in the dust... 
Submillimeter: Planetary systems | Turbulence | Accretion | Protoplanetary disks | Magnetohydrodynamics (MHD) | Instabilities | Accretion disks | PROTOSTELLAR DISKS | accretion, accretion disks | submillimeter: planetary systems | ZERO NET FLUX | turbulence | MHD SIMULATIONS | instabilities | ACCRETION DISKS | DEAD-ZONE | PLANET-FORMING REGIONS | ASTRONOMY & ASTROPHYSICS | ROSSBY-WAVE INSTABILITY | MAGNETOROTATIONAL INSTABILITY | CIRCUMSTELLAR DISKS | protoplanetary disks | magnetohydrodynamics (MHD) | WEAKLY MAGNETIZED DISKS | Magnetohydrodynamics | Turbulent flow | Computer simulation | Protoplanets | Planet formation | Radio telescopes | MHD | Physics | Astrophysics
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3. Full Text Chemistry in Protoplanetary Disks
by Henning, Thomas and Semenov, Dmitry
Chemical Reviews, ISSN 0009-2665, 12/2013, Volume 113, Issue 12, pp. 9016 - 9042
LOW-MASS PROTOSTELLAR | CIRCUMSTELLAR DUST DISKS | SPECTRAL ENERGY-DISTRIBUTIONS | CARLO RADIATIVE-TRANSFER | POLYCYCLIC AROMATIC-HYDROCARBONS | X-RAY IONIZATION | MOLECULAR-HYDROGEN EMISSION | T-TAURI STARS | HERBIG AE/BE STARS | SIZED CARBON GRAINS | CHEMISTRY, MULTIDISCIPLINARY | Planets | Research | Molecular probes | Atmosphere
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4. Full Text Thanatology in protoplanetary discs: The combined influence of Ohmic, Hall, and ambipolar diffusion on dead zones
by Lesur, Geoffroy and Kunz, Matthew W and Fromang, Sébastien
Astronomy and Astrophysics, ISSN 0004-6361, 2014, Volume 566, pp. A56 - np
Protoplanetary discs are poorly ionised due to their low temperatures and high column densities and are therefore subject to three "non-ideal"... 
Magnetohydrodynamics (MHD) | Protoplanetary disks | Instabilities | Stars: formation | Accretion, accretion disks | LINEAR-ANALYSIS | PROTOSTELLAR DISKS | GLOBAL STABILITY | 3-DIMENSIONAL MAGNETOHYDRODYNAMIC SIMULATIONS | accretion, accretion disks | IONIZATION FRACTION | LAYERED ACCRETION | MAGNETOROTATIONAL-INSTABILITY | instabilities | stars: formation | WIND-DRIVEN ACCRETION | T TAURI DISKS | ASTRONOMY & ASTROPHYSICS | protoplanetary disks | magnetohydrodynamics (MHD) | WEAKLY MAGNETIZED DISKS | Ohmic dissipation | Discs | Magnetohydrodynamics | Ambipolar diffusion | MHD | Disks | Hall effect | Accretion disks | Physics | Astrophysics
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5. Full Text Gravitational Instabilities in Circumstellar Disks
by Kratter, Kaitlin and Lodato, Giuseppe
Annual Review of Astronomy and Astrophysics, ISSN 0066-4146, 9/2016, Volume 54, Issue 1, pp. 271 - 311
Star and planet formation are the complex outcomes of gravitational collapse and angular momentum transport mediated by protostellar and protoplanetary disks.... 
star and planet formation | hydrodynamics | accretion disks | Star and planet formation | Hydrodynamics | Accretion disks | PROTOSTELLAR DISKS | SMOOTHED PARTICLE HYDRODYNAMICS | PRE-MAIN-SEQUENCE | BROWN DWARF | SPECTRAL ENERGY-DISTRIBUTIONS | LOW-MASS | GIANT PLANET FORMATION | PROTOPLANETARY DISK | ASTRONOMY & ASTROPHYSICS | COOLING TIME-SCALE | T-TAURI STARS | Mechanics, Celestial
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6. Full Text Unveiling the physical conditions of the youngest disks A warm embedded disk in L1527
by van't Hoff, MLR and Tobin, JJ and Harsono, D and van Dishoeck, EF
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 07/2018, Volume 615, p. A83
Context. Protoplanetary disks have been studied extensively, both physically and chemically, to understand the environment in which planets form. However, the... 
PROTOPLANETARY DISKS | stars: protostars | MOLECULAR CLOUD | SNOW LINE | PROTOSTELLAR SYSTEM | GRAIN-GROWTH | INFALLING ENVELOPE | SPECTRAL ENERGY-DISTRIBUTIONS | ISM: molecules | ASTRONOMY & ASTROPHYSICS | DM-TAU | CIRCUMSTELLAR DISKS | T-TAURI STARS | ISM: individual objects: L1527
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7. Full Text Hall effect controlled gas dynamics in protoplanetary disks. ii. full 3d simulations toward the outer disk
by Bai, Xue-Ning
Astrophysical Journal, ISSN 0004-637X, 01/2015, Volume 798, Issue 2, pp. 84 - 18
We perform three-dimensional stratified shearing-box magnetohydrodynamic (MHD) simulations on the gas dynamics of protoplanetary disks with a net vertical... 
protoplanetary disks | methods: numerical | turbulence | accretion, accretion disks | instabilities | magnetohydrodynamics (MHD) | LINEAR-ANALYSIS | PROTOSTELLAR DISKS | VERTICAL MAGNETIC-FIELD | AMBIPOLAR DIFFUSION | MAGNETOROTATIONAL-INSTABILITY | NONLINEAR EVOLUTION | YOUNG STELLAR OBJECTS | CHEMICAL-PROCESSES | WIND-DRIVEN ACCRETION | ASTRONOMY & ASTROPHYSICS | X-RAY | Magnetohydrodynamics | Simulation | Ohmic | Planet formation | Gas dynamics | Hall effect | Accretion disks | Three dimensional | MAGNETIC FLUX | PROTOPLANETS | MAGNETOHYDRODYNAMICS | THREE-DIMENSIONAL CALCULATIONS | ACCRETION DISKS | LAYERS | ANGULAR MOMENTUM | REFLECTION | SHEAR | NMR IMAGING | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | EQUILIBRIUM | TURBULENCE | HALL EFFECT
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8. Full Text Hall-effect-controlled gas dynamics in protoplanetary disks. I. wind solutions at the inner disk
by Bai, Xue-Ning
Astrophysical Journal, ISSN 0004-637X, 08/2014, Volume 791, Issue 2, pp. 137 - 22
The gas dynamics of protoplanetary disks (PPDs) is largely controlled by non-ideal magnetohydrodynamic (MHD) effects including Ohmic resistivity, the Hall... 
protoplanetary disks | methods: numerical | turbulence | instabilities | magnetohydrodynamics (MHD) | SURFACE-LAYER ACCRETION | AMBIPOLAR DIFFUSION | MAGNETOROTATIONAL-INSTABILITY | NONLINEAR EVOLUTION | PROTOSTELLAR ACCRETION DISCS | UNSPLIT GODUNOV METHOD | DRIVEN ACCRETION | ASTRONOMY & ASTROPHYSICS | X-RAY IONIZATION | T-TAURI DISKS | WEAKLY MAGNETIZED DISKS | Stellar winds | Magnetohydrodynamics | Protoplanets | Planet formation | Gas dynamics | MHD | Hall effect | Accretion disks | MAGNETIC FIELDS | MATHEMATICAL SOLUTIONS | INSTABILITY | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | PROTOPLANETS | MAGNETOHYDRODYNAMICS | TURBULENCE | HALL EFFECT | SIMULATION | STRESSES
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9. Full Text Can giant planets form by gravitational fragmentation of discs? Radiative hydrodynamic simulations of the inner disc region (less than or similar to 40 AU)
by Stamatellos, D and Whitworth, AP
ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 03/2008, Volume 480, Issue 3, pp. 879 - 887
Context. Gravitational fragmentation has been proposed as a mechanism for the formation of giant planets in close orbits around solar-type stars. However, it... 
planets and satellites : formation | INSTABILITY | radiative transfer | STABILITY | THERMAL REGULATION | STAR-FORMATION | hydrodynamics | SMOOTHED PARTICLE HYDRODYNAMICS | accretion, accretion discs | instabilities | UNSTABLE PROTOPLANETARY DISKS | PROTOSTELLAR COLLAPSE | EVOLUTION | stars : planetary systems : protoplanetary discs | ACCRETION DISCS | ASTRONOMY & ASTROPHYSICS | MOLECULAR CLOUD CORES
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10. Full Text Global simulations of protoplanetary disks with net magnetic flux: I. Non-ideal MHD case
by Béthune, William and Lesur, Geoffroy and Ferreira, Jonathan
Astronomy and Astrophysics, ISSN 0004-6361, 04/2017, Volume 600, p. A75
Context. The planet-forming region of protoplanetary disks is cold, dense, and therefore weakly ionized. For this reason, magnetohydrodynamic (MHD) turbulence... 
stars: formation | protoplanetary disks | turbulence | accretion, accretion disks | magnetohydrodynamics (MHD) | PROTOSTELLAR DISKS | 3-DIMENSIONAL MAGNETOHYDRODYNAMIC SIMULATIONS | AMBIPOLAR DIFFUSION | MAGNETOROTATIONAL-INSTABILITY | NONLINEAR EVOLUTION | DRIVEN ACCRETION | ASTRONOMY & ASTROPHYSICS | ACCRETION-EJECTION STRUCTURES | YOUNG STARS | VERTICAL SHEAR INSTABILITY | MULTIFLUID SIMULATIONS | Magnetohydrodynamics | Accretion | Turbulent flow | Computer simulation | Planet formation | Heating | Magnetic fields | Accretion disks | Physics - Earth and Planetary Astrophysics
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