activity
20172022
most citedDynamical evolution of star-forming regions: III. Unbound stars and predictions for Gaia

32 citations · 76 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2022★ 12 cited

Quantifying kinematic substructure in star-forming regions with statistical tests of spatial autocorrelation

Becky Arnold, Nicholas J. Wright, Richard J. Parker

We investigate whether spatial-kinematic substructure in young star-forming regions can be quantified using Moran's statistic. Its presence in young star clusters would provide…

astro-ph.SR2020★ 5 cited

The velocity structure of Cygnus OB2

Becky Arnold, Simon P. Goodwin, Nick J. Wright

The kinematic structure of the Cygnus OB2 association is investigated. No evidence of expansion or contraction is found at any scale within the region. Stars that are within …

astro-ph.SR2019★ 32 cited

Dynamical evolution of star-forming regions: III. Unbound stars and predictions for Gaia

Christina Schoettler, Richard J. Parker, Becky Arnold +3

We use -body simulations to probe the early phases of the dynamical evolution of star-forming regions and focus on mass and velocity distributions of unbound stars. In this para…

astro-ph.SR2018★ 5 cited

A method to analyse velocity structure

Becky Arnold, Simon Goodwin

We present a new method of analysing and quantifying velocity structure in star forming regions suitable for the rapidly increasing quantity and quality of stellar position-velocit…

astro-ph.GA2017★ 22 cited

How do binary clusters form?

Becky Arnold, Simon P. Goodwin, Daniel W. Griffiths +1

Approximately 10 per cent of star clusters are found in pairs, known as binary clusters. We propose a mechanism for binary cluster formation; we use N-body simulations to show that…