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The circles represent different infall rates of˙Minfall =5×10 −10, 5×10 −9, 5×10 −8, 5×10 −7 M⊙yr−1, respectively, in order of increasing circle size · 2025

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astro-ph.EP 1

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2026 1

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From streamers to stars: overcoming mass loss in protoplanetary disks

astro-ph.EP · 2026-05-26 · unverdicted · novelty 4.0

1D long-term simulations show that MHD disk winds are required to sustain stellar accretion from late infall in compact protoplanetary disks when no effective infall torque is present, as photoevaporation removes most gas and viscosity causes excessive spreading.

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  • From streamers to stars: overcoming mass loss in protoplanetary disks astro-ph.EP · 2026-05-26 · unverdicted · none · ref 2

    1D long-term simulations show that MHD disk winds are required to sustain stellar accretion from late infall in compact protoplanetary disks when no effective infall torque is present, as photoevaporation removes most gas and viscosity causes excessive spreading.