activity
20032026
most citedMagnetic Field Generation in Collisionless Shocks; Pattern Growth and Transport

233 citations · 3.7k across the 79 of their papers we have counts for

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Showing astro-ph.EPShow all

14 papers · 1 filter

astro-ph.EP2026

Planetesimal formation facilitated by streaming instability in weak pressure bumps

Magnus S. Sørensen-Taylor, Anders Johansen, Troels Haugbølle

Planetesimal formation via the streaming instability of small pebbles in protoplanetary discs requires enhanced solid concentrations relative to the solar metallicity, $Z\simeq 0.0…

astro-ph.EP2026

Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs

Christian Granzow Holm, Michiel Lambrechts, Michael Kuffmeier +3

Protoplanetary discs evolve around newly-formed stars through an interplay of infall from surrounding turbulent cloud material, accretion towards the young star, and outflow driven…

astro-ph.EP2025★ 1 cited

Interstellar Ices as Carriers of Supernova Material to the Early Solar System

Martin Bizzarro, Martin Schiller, Jesper Holst +10

Planetary materials show systematic variations in their nucleosynthetic isotope compositions that resonate with orbital distance. The origin of this pattern remains debated, limiti…

astro-ph.EP2024

Thousands of planetesimals: Simulating the streaming Instability in very large computational domains

Urs Schäfer, Anders Johansen, Troels Haugbølle +1

The streaming instability is a mechanism whereby pebble-sized particles in protoplanetary discs spontaneously come together in dense filaments, which collapse gravitationally to fo…

astro-ph.EP2022

Natural separation of two primordial planetary reservoirs in an expanding solar protoplanetary disk

Beibei Liu, Anders Johansen, Michiel Lambrechts +2

Meteorites display an isotopic composition dichotomy between non-carbonaceous (NC) and carbonaceous (CC) groups, indicating that planetesimal formation in the solar protoplanetary…

astro-ph.EP2021★ 34 cited

Hybrid accretion of carbonaceous chondrites by radial transport across the Jupiter barrier

Elishevah van Kooten, Martin Schiller, Frederic Moynier +3

Understanding the origin of chondritic components and their accretion pathways is critical to unravel the magnitude of mass transport in the protoplanetary disk, the accretionary h…