activity
20172022
most citedPebbles versus planetesimals: the outcomes of population synthesis models

52 citations · 242 across the 7 of their papers we have counts for

collaborators

12 papers

astro-ph.EP202219 cited

Dusty circumbinary discs: inner cavity structures and stopping locations of migrating planets

Gavin A. L. Coleman, Richard P. Nelson, Amaury H. M. J. Triaud

We present the results of two-fluid hydrodynamical simulations of circumbinary discs consisting of gas and dust, with and without embedded planets, to examine the influence of the…

astro-ph.EP202126 cited

From Dust to Planets I: Planetesimal and Embryo Formation

Gavin A. L. Coleman

Planet formation models begin with proto-embryos and planetesimals already fully formed, missing out a crucial step, the formation of planetesimals/proto-embryos. In this work, we…

astro-ph.EP202126 cited

In situ formation of hot Jupiters with companion super-Earths

Sanson T. S. Poon, Richard P. Nelson, Gavin A. L. Coleman

Observations have confirmed the existence of multiple-planet systems containing a hot Jupiter and smaller planetary companions. Examples include WASP-47, Kepler-730, and TOI-1130.…

astro-ph.SR202022 cited

Peter Pan Discs: finding Neverland's parameters

Gavin A. L. Coleman, Thomas J. Haworth

Peter Pan discs are a recently discovered class of long-lived discs around low-mass stars that survive for an order of magnitude longer than typical discs. In this paper we use dis…

astro-ph.EP202052 cited

Pebbles versus planetesimals: the outcomes of population synthesis models

Natacha Brügger, Remo Burn, Gavin Coleman +2

In the core accretion scenario, a massive core forms first and then accretes an envelope. When discussing how this core forms some divergences appear. First scenarios of planet for…

astro-ph.EP2020

The CARMENES search for exoplanets around M dwarfs. Characterization of the nearby ultra-compact multiplanetary system YZ Ceti

S. Stock, J. Kemmer, S. Reffert +38

The nearby ultra-compact multiplanetary system YZ Ceti consists of at least three planets. The orbital period of each planet is the subject of discussion in the literature due to s…