1.3k citations · 1.3k across the 12 of their papers we have counts for
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From dust to planets -- II. Effects of wide binary companions and external photoevaporation on planetesimal and embryo formation
Gavin A. L. Coleman
More than half of Solar-type stars are found in binary systems. The numbers of exoplanets within binary systems in s-type orbits now numbers over 700. However, whilst the numbers h…
Formation of multi-planetary systems via pebble accretion in externally photoevaporating discs in stellar clusters
Lin Qiao, Gavin A. L. Coleman, Thomas J. Haworth
In this paper, we investigate how external photo-evaporation influences the formation, dynamical evolution and the resultant planetary architecture of multi-planet systems born in…
Using simultaneous mass accretion and external photoevaporation rates for d203-504 to constrain disc evolution processes
Gavin A. L. Coleman, Thomas J. Haworth, Ilane Schroetter +1
We cannot understand planet formation without understanding disc evolutionary processes. However, there is currently ambiguity about how protoplanetary discs transport angular mome…
How the gradient of versus UV field strength yields insights into the ages of protoplanetary disc populations
Gavin A. L. Coleman, Sierk E. van Terwisga
FUV radiation from massive stars launch photoevaporative winds from the outer regions of protoplanetary discs around other stars, removing gas and dust. Observations have identifie…
Runaway origins of a disc mass gradient in Orionis
Gavin A. L. Coleman, Thomas J. Haworth, Jinyoung Serena Kim
Radiation from massive stars is known to significantly affect the evolution of protoplanetary discs around surrounding stars by driving external photoevaporative winds. Typically m…
The observable impact of runaway OB stars on protoplanetary discs
Gavin A. L. Coleman, Jinyoung Serena Kim, Thomas J. Haworth +2
UV radiation from OB stars can drive ``external'' photoevaporative winds from discs in clusters, that have been shown to be important for disc evolution and planet formation. Howev…