activity
20062026
most citedContacts of Water Ice in Protoplanetary Disks - Laboratory Experiments

189 citations · 2.3k across the 79 of their papers we have counts for

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Showing 2020Show all

7 papers · 1 filter

astro-ph.EP2020★ 8 cited

Destruction of eccentric planetesimals by ram pressure and erosion

Tunahan Demirci, Niclas Schneider, Jens Teiser +1

Small, pebble-sized objects and large bodies of planetesimal size both play important roles in planet formation. They form the evolutionary steps of dust growth in their own respec…

astro-ph.EP2020★ 8 cited

Cosmic radiation does not prevent collisional charging in (Pre)-Planetary Atmospheres

Felix Jungmann, Tetyana Bila, Laura Kleinert +8

In (pre)-planetary environments, dust and sand grains regularly collide. They electrically charge and discharge during these events. In this work, we study if cosmic radiation has…

astro-ph.EP2020★ 7 cited

Accretion of eroding pebbles and planetesimals in planetary envelopes

Tunahan Demirci, Gerhard Wurm

Wind erosion is a destructive mechanism that completely dissolves a weakly bound object like a planetesimal into its constituent particles, if the velocity relative to the ambient…

astro-ph.EP2020★ 13 cited

Laboratory Impact Splash Experiments to Simulate Asteroid Surfaces

Tabea Bogdan, Jonathan E. Kollmer, Jens Teiser +2

Granular material that is bound by the low gravity of a small asteroid is mobilized by slow velocity impacts. These splashes generated by impacts might play an important role in sc…

astro-ph.EP2020★ 26 cited

Composition and Size Dependent Sorting in Preplanetary Growth: Seeding the Formation of Mercury-like Planets

Maximilian Kruss, Gerhard Wurm

In an earlier work, we found that large metallic iron fractions in dust aggregates and strong magnetic fields boost preplanetary growth. This sets an initial bias for the formation…

astro-ph.EP2020★ 21 cited

Planetesimals in Rarefied Gas: Wind Erosion in Slip Flow

Tunahan Demirci, Niclas Schneider, Tobias Steinpilz +3

A planetesimal moves through the gas of its protoplanetary disc where it experiences a head wind. Though the ambient pressure is low, this wind can erode and ultimately destroy the…