530 citations · 6k across the 86 of their papers we have counts for
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New evidence for wet accretion of inner solar system planetesimals from meteorites Chelyabinsk andBenenitra
Ziliang Jin, Maitrayee Bose, Tim Lichtenberg +1
We investigated the hydrogen isotopic compositions and water contents of pyroxenes in two recent ordinary chondrite falls, namely, Chelyabinsk (2013 fall) and Benenitra (2018 fall)…
Why do M dwarfs have more transiting planets?
Gijs D. Mulders, Joanna Drążkowska, Nienke van der Marel +2
We propose a planet formation scenario to explain the elevated occurrence rates of transiting planets around M dwarfs compared to sun-like stars discovered by Kepler. We use a pebb…
Linking Outer Disk Pebble Dynamics and Gaps to Inner Disk Water Enrichment
A. Kalyaan, P. Pinilla, S. Krijt +2
Millimeter continuum imaging of protoplanetary disks reveals the distribution of solid particles and the presence of substructures (gaps and rings) beyond 5-10 au, while infrared (…
If you like C/O variations, you should have put a ring on it
Nienke van der Marel, Arthur Bosman, Sebastiaan Krijt +2
The C/O-ratio as traced with CH emission in protoplanetary disks is fundamental for constraining the formation mechanisms of exoplanets and our understanding of volatile deplet…
The Mass Budgets and Spatial Scales of Exoplanet Systems and Protoplanetary Disks
Gijs D. Mulders, Ilaria Pascucci, Fred J. Ciesla +1
Planets are born from disks of gas and dust, and observations of protoplanetary disks are used to constrain the initial conditions of planet formation. However, dust mass measureme…
A stellar mass dependence of structured disks: a possible link with exoplanet demographics
Nienke van der Marel, Gijs Mulders
Gaps in protoplanetary disks have long been hailed as signposts of planet formation. However, a direct link between exoplanets and disks remains hard to identify. We present a larg…