activity
20152022
most citedHints for a Turnover at the Snow Line in the Giant Planet Occurrence Rate

266 citations · 1.2k across the 18 of their papers we have counts for

collaborators

35 papers

astro-ph.EP202237 cited

The Demographics of Kepler's Earths and super-Earths into the Habitable Zone

Galen J. Bergsten, Ilaria Pascucci, Gijs D. Mulders +2

Understanding the occurrence of Earth-sized planets in the habitable zone of Sun-like stars is essential to the search for Earth analogues. Yet a lack of reliable Kepler detections…

astro-ph.EP202170 cited

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…

astro-ph.EP202125 cited

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…

astro-ph.EP20211 cited

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…

astro-ph.EP2021

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…

astro-ph.SR20201 cited

X-Shooter survey of disk accretion in Upper Scorpius I. Very high accretion rates at age>5 Myr

C. F. Manara, A. Natta, G. P. Rosotti +14

Determining the mechanisms that drive the evolution of protoplanetary disks is a necessary step to understand how planets form. Here we measured the mass accretion rate for young s…