activity
20092026
most citedUsing the minimum spanning tree to trace mass segregation

234 citations · 234 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2026

Bridging the gap between stars and planets

Aina Palau, Dimitris Stamatellos, Matthew Bate +58

The formation mechanisms of brown dwarfs (BDs) and free-floating planets (FFPs) are poorly constrained. The two main competing scenarios include the star-like scenario, where these…

astro-ph.EP2026

White dwarf planets in star clusters: gravitational scattering versus mass-loss effects

Richard J. Parker, Dimitri Veras

White dwarfs are unique laboratories for understanding the formation, evolution and survivability of planetary systems. Post-main sequence mass-loss will change planetary orbital p…

astro-ph.EP2026

Planet or brown dwarf? Constraints on the formation of H-type objects in IC348

Richard J. Parker, Catarina Alves de Oliveira

The formation mechanism(s) of substellar objects, such as brown dwarfs and free-floating planets, remains an ongoing puzzle in stellar and planetary physics. Recent observational a…

astro-ph.SR2025

Hidden binaries in star-forming regions

Mary H. Rawcliffe, Nathan Griffiths-Janvier, Richard J. Parker

A significant fraction of, and possibly all, stars form in binary or multiple systems. For Solar-mass stars in the Galactic field, the distribution of orbital separations is log-no…

astro-ph.SR2025

Can planet-planet binaries survive in star-forming regions?

Richard J. Parker, Simon P. Goodwin, Jessica L. Diamond

Significant numbers of free-floating planetary-mass objects have been discovered in nearby star-forming regions by the James Webb Space Telescope, including a substantial number (4…

astro-ph.GA2009★ 234 cited

Using the minimum spanning tree to trace mass segregation

Richard J. Allison, Simon P. Goodwin, Richard J. Parker +3

We present a new method to detect and quantify mass segregation in star clusters. It compares the minimum spanning tree (MST) of massive stars with that of random stars. If mass se…