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20152026
most citedZoom-Simulations of Protoplanetary Disks starting from GMC scales

124 citations · 1.1k across the 33 of their papers we have counts for

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20 papers · 1 filter

astro-ph.SR2026

Stellar age is not disk age

M. Kuffmeier, A. Winter, A. Kuznetsova +2

Disk fractions in star-forming clusters decline with stellar age, and are routinely read as the lifetime distribution of primordial protoplanetary disks. We argue that this reading…

astro-ph.SR2025

Preferential accretion of binary stars

Daniel Dalsgaard, Michael Kuffmeier, Troels Haugbølle

The attracting properties of gravity enable matter present in cores to collapse into stars with seven orders of magnitude change in space and time making modelling of star formatio…

astro-ph.SR2024★ 1 cited

Magnetohydrodynamical modeling of star-disk formation: from isolated spherical collapse towards incorporation of external dynamics

M. Kuffmeier

The formation of protostars and their disks has been understood as the result of the gravitational collapse phase of an accumulation of dense gas that determines the mass reservoir…

astro-ph.SR2024★ 19 cited

Constraints on the (re-)orientation of star-disk systems through infall

M. Kuffmeier, J. E. Pineda, D. Segura-Cox +1

It has been consensus that star-disk systems accrete most of their mass and angular momentum during the collapse of a prestellar core, such that the rotational direction of a syste…

astro-ph.SR2024★ 10 cited

Feasibility of detecting shadows in disks induced by infall

A. Krieger, M. Kuffmeier, S. Reissl +3

Observations performed with high-resolution imaging techniques revealed the existence of shadows in circumstellar disks that can be explained by the misalignment of an inner with r…

astro-ph.SR2024

TIPSY: Trajectory of Infalling Particles in Streamers around Young stars. Dynamical analysis of the streamers around S CrA and HL Tau

Aashish Gupta, Anna Miotello, Jonathan P. Williams +3

Context. Elongated trails of infalling gas, often referred to as "streamers," have recently been observed around young stellar objects (YSOs) at different evolutionary stages. This…