Context. The dead zone outer edge corresponds to the transition from the magnetically dead to the magnetorotational instability (MRI) active regions in the outer protoplanetary disk midplane. It has been previously hypothesized to be a prime location for dust particle trapping. A more consistent approach to access such an idea has yet to be developed, since the interplay between dust evolution and MRI-driven accretion over millions of years has been poorly understood. Aims. We provide an important step toward a better understanding of the MRI- dust coevolution in protoplanetary disks. In this pilot study, we present a proof of concept that dust evolution ultimately plays a crucial role in the MRI activity. Methods. First, we study how a fix...
Aims. We study the dynamics and growth of dust particles in circumstellar disks of different masses ...
Recent surveys have revealed that protoplanetary discs typically have dust masses that appear to be ...
International audienceContext. Magnetohydrodynamic (MHD) turbulence plays a crucial role in the dust...
Context. The transition between magnetorotational instability (MRI)-active and magnetically dead reg...
Aims. Accretion bursts triggered by the magnetorotational instability (MRI) in the innermost disk re...
Aims. Accretion bursts triggered by the magnetorotational instability (MRI) in the innermost disk re...
Magnetorotational instability (MRI) is the most promising mechanism behind accretion in low-mass pro...
Previous models of dust growth in protoplanetary disks considered either uniformly laminar or turbul...
As an initial investigation into the long-term evolution of protostellar disks, we explore the condi...
As an initial investigation into the long-term evolution of protostellar disks, we explore the condi...
Context. The poorly-ionized interior of the protoplanetary disk or ââ¬Ådead zoneââ¬Â is the lo...
We consider the dynamics of dust and gas during the clearing of protoplanetary discs. We work within...
Context. Current models of the size- and radial evolution of dust in protoplanetary disks generally ...
Recent surveys have revealed that protoplanetary discs typically have dust masses that appear to be ...
Context. Regions of low ionisation where the activity of the magneto-rotational instability is suppr...
Aims. We study the dynamics and growth of dust particles in circumstellar disks of different masses ...
Recent surveys have revealed that protoplanetary discs typically have dust masses that appear to be ...
International audienceContext. Magnetohydrodynamic (MHD) turbulence plays a crucial role in the dust...
Context. The transition between magnetorotational instability (MRI)-active and magnetically dead reg...
Aims. Accretion bursts triggered by the magnetorotational instability (MRI) in the innermost disk re...
Aims. Accretion bursts triggered by the magnetorotational instability (MRI) in the innermost disk re...
Magnetorotational instability (MRI) is the most promising mechanism behind accretion in low-mass pro...
Previous models of dust growth in protoplanetary disks considered either uniformly laminar or turbul...
As an initial investigation into the long-term evolution of protostellar disks, we explore the condi...
As an initial investigation into the long-term evolution of protostellar disks, we explore the condi...
Context. The poorly-ionized interior of the protoplanetary disk or ââ¬Ådead zoneââ¬Â is the lo...
We consider the dynamics of dust and gas during the clearing of protoplanetary discs. We work within...
Context. Current models of the size- and radial evolution of dust in protoplanetary disks generally ...
Recent surveys have revealed that protoplanetary discs typically have dust masses that appear to be ...
Context. Regions of low ionisation where the activity of the magneto-rotational instability is suppr...
Aims. We study the dynamics and growth of dust particles in circumstellar disks of different masses ...
Recent surveys have revealed that protoplanetary discs typically have dust masses that appear to be ...
International audienceContext. Magnetohydrodynamic (MHD) turbulence plays a crucial role in the dust...