activity
20172022
most citedPlanet population synthesis driven by pebble accretion in cluster environments

101 citations · 185 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP20228 cited

The role of density perturbation on planet formation by pebble accretion

Geoffrey Andama, Nelson Ndugu, Simon . K. Anguma +1

Protoplanetary discs exhibit a diversity of gaps and rings of dust material, believed to be a manifestation of pressure maxima commonly associated with an ongoing planet formation…

astro-ph.EP202213 cited

Planet population synthesis: The role of stellar encounters

Nelson Ndugu, Oyirwoth Patrick Abedigamba, Geoffrey Andama

Depending on the stellar densities, protoplanetary discs in stellar clusters undergo background heating, disc truncation-driven by stellar encounter, and photo-evaporation. Disc tr…

astro-ph.EP202029 cited

Probing the impact of varied migration and gas accretion rates for the formation of giant planets in the pebble accretion scenario

Nelson Ndugu, Bertram Bitsch, Alessandro Morbidelli +2

The final orbital position of growing planets is determined by their migration speed, which is essentially set by the planetary mass. Small mass planets migrate in type I migration…

astro-ph.EP201934 cited

Are the observed gaps in protoplanetary discs caused by growing planets?

Nelson Ndugu, Bertram Bitsch, Edward Jurua

Recent detailed observations of protoplanetary discs revealed a lot of sub-structures which are mostly ring-like. One interpretation is that these rings are caused by growing plane…

astro-ph.EP2017101 cited

Planet population synthesis driven by pebble accretion in cluster environments

Nelson Ndugu, Bertram Bitsch, Edward Jurua

The evolution of protoplanetary discs embedded in stellar clusters depends on the age and the stellar density in which they are embedded. Stellar clusters of young age and high ste…