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Astronomy and astrophysics (Berlin), ISSN 0004-6361, 05/2019, Volume 625, p. A66
Journal Article
Astronomy and astrophysics (Berlin), 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 continuum emission... 
Submillimeter: Planetary systems | Turbulence | Accretion | Protoplanetary disks | Magnetohydrodynamics (MHD) | Instabilities | Accretion disks | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Magnetohydrodynamics | Turbulent flow | Computer simulation | Protoplanets | Planet formation | Radio telescopes | MHD | Physics | Astrophysics
Journal Article
Annual review of astronomy and astrophysics, ISSN 0066-4146, 9/2011, Volume 49, Issue 1, pp. 195 - 236
Protoplanetary disks are quasi-steady structures whose evolution and dispersal determine the environment for planet formation... 
pre-main-sequence stars | accretion | protoplanetary disks | Protoplanetary disks | Pre-main-sequence stars | Accretion | Astrophysics | Research | Planetary rings | Properties | Observations | Dynamics | Theory | Star & galaxy formation | Magnetization | Planet formation | Ionization | Planetary evolution | Stars | Disks | Planetary probes
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2016, Volume 589, p. A87
Context. Recent observations have revealed organised structures in protoplanetary discs, such as axisymmetric rings or horseshoe concentrations, evocative of large-scale vortices... 
Magnetohydrodynamics (MHD) | stars: formation | Turbulence | Protoplanetary disks | Accretion, accretion disks | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Turbulent flow | Computational fluid dynamics | Protoplanets | Planet formation | Vortices | Fluid flow | Hall effect | Physics - Earth and Planetary Astrophysics
Journal Article