Multiwavelength modelling of the ß Leo debris disc: one, two or three planetesimal populations?? Modelling the ß Leo debris disc (2011)

First Author: Churcher L

Attributed to: Research in Theoretical Astronomy 2009-2014 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2011.19341.x

Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2011.19341.x

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 3