Self-consistent modelling of line-driven hot-star winds with Monte Carlo radiation hydrodynamics (2015)

First Author: Noebauer U
Attributed to:  PATT Linked Grant for observational astrophysics at QUB: 2014 - 2016 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stv1849

Publication URI: http://dx.doi.org/10.1093/mnras/stv1849

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 3