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Astronomy and astrophysics (Berlin), ISSN 1432-0746, 2019, Volume 633, p. A21
Context. Photoevaporation and magnetically driven winds are two independent mechanisms that remove mass from protoplanetary disks. In addition to accretion,... 
magnetic fields | SHEAR INSTABILITY | FAR-ULTRAVIOLET | hydrodynamics | MHD SIMULATIONS | RADIATION | DISPERSAL | accretion | ASTRONOMY & ASTROPHYSICS | ACCRETION-EJECTION STRUCTURES | X-RAY | STELLAR | CIRCUMSTELLAR DISKS | MAGNETOROTATIONAL INSTABILITY | protoplanetary disks | magnetohydrodynamics (MHD) | accretion disks
Journal Article
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2016, Volume 591, p. A36
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2009, Volume 400, Issue 2, pp. 820 - 834
Journal Article
Astrophysical Journal, ISSN 0004-637X, 02/2016, Volume 818, Issue 2, p. 152
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2020, Volume 494, Issue 4, pp. 6103 - 6119
The vertical temperature structure of a protoplanetary disc bears on several processes relevant to planet formation, such as gas and dust grain chemistry, ice lines, and convection... 
LOCAL SHEAR INSTABILITY | LINEAR-ANALYSIS | YOUNG OBJECTS | radiation: dynamics | protoplanetary discs | ICE LINES | MHD | AMBIPOLAR DIFFUSION | accretion, accretion discs | CENTRIFUGALLY DRIVEN WINDS | ASTRONOMY & ASTROPHYSICS | ACCRETION-EJECTION STRUCTURES | MAGNETOROTATIONAL INSTABILITY | IONIZATION STATE | WEAKLY MAGNETIZED DISKS
Journal Article