📣 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.

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