623 citations · 2.4k across the 29 of their papers we have counts for
29 papers
A pebble accretion model for the formation of the terrestrial planets in the Solar System
Anders Johansen, Thomas Ronnet, Martin Bizzarro +4
Pebbles of millimeter sizes are abundant in protoplanetary discs around young stars. Chondrules inside primitive meteorites - formed by melting of dust aggregate pebbles or in impa…
The structure and characteristic scales of molecular clouds
Sami Dib, Sylvain Bontemps, Nicola Schneider +8
The structure of molecular clouds (MCs) holds important clues on the physical processes that lead to their formation and subsequent evolution. While it is well established that tur…
Early formation of planetary building blocks inferred from Pb isotopic ages of chondrules
Jean Bollard, James N. Connelly, Martin J. Whitehouse +6
The most abundant components of primitive meteorites (chondrites) are millimeter-sized glassy spherical chondrules formed by transient melting events in the solar protoplanetary di…
Particle-in-cell Simulations of Global Relativistic Jets with Helical Magnetic Fields
Ioana Duţan, Ken-Ichi Nishikawa, Yosuke Mizuno +11
We study the interaction of relativistic jets with their environment, using 3-dimensional relativistic particle-in-cell simulations for two cases of jet composition: (i) electron-p…
Supernova Driving. I. The Origin of Molecular Cloud Turbulence
Paolo Padoan, Liubin Pan, Troels Haugboelle +1
Turbulence is ubiquitous in molecular clouds (MCs), but its origin is still unclear because MCs are usually assumed to live longer than the turbulence dissipation time. Interstella…
Zooming in on the Formation of Protoplanetary Disks
A. Nordlund, T. Haugboelle, M. Kuffmeier +2
We use the adaptive mesh refinement code RAMSES to model the formation of protoplanetary disks in realistic star formation environments. The resolution scales over up to 29 powers…