📣 Help Shape the Future of UKRI's Gateway to Research (GtR)

We're improving UKRI's Gateway to Research and are seeking your input! If you would be interested in being interviewed about the improvements we're making and to have your say about how we can make GtR more user-friendly, impactful, and effective for the Research and Innovation community, please email gateway@ukri.org.

Modelling the structure of star clusters with fractional Brownian motion (2018)

First Author: Lomax O

Attributed to: A programme of Astrophysics, Cosmology and Technology in Cardiff 2013-2016 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/sty1788

Publication URI: http://dx.doi.org/10.1093/mnras/sty1788

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 1