activity
20172026
most citedPlanet population synthesis driven by pebble accretion in cluster environments

101 citations · 357 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2026

High-precision K2/TESS Photometry and HERMES Spectroscopy of Four Bright Field Stars

Otto Trust, Santosh Joshi, Benard Nsamba +13

Space-based photometry from K2 and TESS, coupled with high-resolution spectroscopy, provides a unique opportunity to re-examine the variability and chemical nature of four bright s…

astro-ph.SR2023★ 6 cited

High-precision photometric and high-resolution spectroscopic characterisation of HD 180347

Otto Trust, Lyudmila Mashonkina, Edward Jurua +3

We report the analysis of high-precision space-based photometric and high-resolution spectroscopic observations of HD 180347. The high-quality light curves from the Transiting Exop…

astro-ph.EP2022★ 8 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.EP2021★ 14 cited

Planetary core formation via multi-species pebble accretion

Geoffrey Andama, Nelson Ndugu, Simon Katrini Anguma +1

In the general classical picture of pebble-based core growth, planetary cores grow by accretion of single pebble species. The growing planet may reach the so-called pebble isolatio…

astro-ph.SR2021★ 12 cited

Study of Chemically Peculiar Stars-I : High-resolution Spectroscopy and K2 Photometry of Am Stars in the Region of M44

Santosh Joshi, Otto Trust, E. Semenko +30

We present a study based on the high-resolution spectroscopy and K2 space photometry of five chemically peculiar stars in the region of the open cluster M44. The analysis of the hi…

astro-ph.SR2021★ 16 cited

Rotation and spots in normal A and Am/Fm stars

Otto Trust, Edward Jurua, Peter De Cat +1

Frequency analysis of long-term ultra-precise photometry can lead to precise values of rotation frequencies of rotating stars with ``hump and spike'' features in their periodograms…