7 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Lund UniversitySE5 papers
- Geocenter DenmarkDK4 papers
- Max Planck Institute for AstronomyDE3 papers
- Centre National de la Recherche ScientifiqueFR2 papers
- ETH ZurichCH2 papers
- Institute of AstronomyRU2 papers
- Institute of Astrophysics and Space SciencesPT2 papers
- Leiden UniversityNL2 papers
- National Central UniversityTW2 papers
- University of California, BerkeleyUS2 papers
- University of CopenhagenDK2 papers
- Arcetri Astrophysical ObservatoryIT1 paper
5 papers · 1 filter
The Baryonic Faber-Jackson Relation and Fundamental Plane of Galaxy Groups, Elliptical Galaxies, and Dwarf Galaxies
Yong Tian, Federico Lelli, Marcel S. Pawlowski +7
The baryonic Faber-Jackson relation (BFJR) links the baryonic mass of pressure-supported systems to their mean velocity dispersion. For elliptical galaxies, the BFJR is thought to…
Exploring the conditions for forming planetesimals by the streaming instability and planetary systems by pebble accretion
Anders Johansen, Wladimir Lyra
The streaming instability and pebble accretion are two physical mechanisms with demonstrated potentials to drive, respectively, the formation of planetesimals and the growth of pla…
How leaky? A large parameter study of leaky dust traps to quantify the transport of pebbles and ice in protoplanetary discs
Adrien Houge, Anders Johansen, Andrea Banzatti +1
In protoplanetary discs, the presence of dust traps can significantly alter the transport of solids from the outer to the inner regions, and hence they are often invoked as an expl…
A break in planet occurrence near the pebble isolation mass should be observable by the Roman microlensing survey
Claudia Danti, Michiel Lambrechts, Hannah Diamond-Lowe
Microlensing detections are uniquely well-suited to probing the population of planets outside the water iceline, down to planetary masses comparable to the Earth. Here, we perform…
Interior dynamics of envelopes around disk-embedded planets
Ayumu Kuwahara, Michiel Lambrechts
In the core accretion scenario, forming planets start to acquire gaseous envelopes while accreting solids. Conventional one-dimensional models assume envelopes to be static and iso…