activity
20092017
most citedEvidence for the formation of comet 67P/Churyumov-Gerasimenko through gravitational collapse of a bound clump of pebbles

190 citations · 420 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2017★ 190 cited

Evidence for the formation of comet 67P/Churyumov-Gerasimenko through gravitational collapse of a bound clump of pebbles

Jürgen Blum, Bastian Gundlach, Maya Krause +19

The processes that led to the formation of the planetary bodies in the Solar System are still not fully understood. Using the results obtained with the comprehensive suite of instr…

astro-ph.EP2011★ 95 cited

Thermal conductivity measurements of porous dust aggregates: I. Technique, model and first results

Maya Krause, Jürgen Blum, Yuri V. Skorov +1

We present a non-invasive technique for measuring the thermal conductivity of fragile and sensitive materials. In the context of planet formation research, the investigation of the…

astro-ph.EP2010★ 32 cited

Numerical Simulations of Highly Porous Dust Aggregates in the Low-Velocity Collision Regime

Ralf J. Geretshauser, Roland Speith, Carsten Güttler +2

A highly favoured mechanism of planetesimal formation is collisional growth. Single dust grains, which follow gas flows in the protoplanetary disc, hit each other, stick due to van…

astro-ph.EP2009★ 102 cited

The Physics of Protoplanetesimal Dust Agglomerates. IV. Towards a Dynamical Collision Model

Carsten Güttler, Maya Krause, Ralf J. Geretshauser +2

Recent years have shown many advances in our knowledge of the collisional evolution of protoplanetary dust. Based on a variety of dust-collision experiments in the laboratory, our…

astro-ph.EP2009★ 1 cited

Towards a Dynamical Collision Model of Highly Porous Dust Aggregates

Carsten Güttler, Maya Krause, Ralf J. Geretshauser +2

In the recent years we have performed various experiments on the collision dynamics of highly porous dust aggregates and although we now have a comprehensive picture of the microme…