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Semi-analytic modelling of the dynamics and outflows of stars with powerful winds.

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ck-motion

Last updated: 15.10.2019
Version: 0.01
Python version: 3.6

Contents

Overview
Publication

Overview

ck-motion is a repository containing the code for analysing the outflows and dynamics of binary star components exhibiting powerful winds. The core algorithm is a semi-analytical model which encapsulates the dynamics associated with extended emission, encoding the net velocity field of the out-flowing gas in terms of a convolution of past motion due to the finite flow speed of the wind.

/ckm : the modelling code
/test : unit testing
/analytics : example usage of the ckm API

Publication

The associated paper is available at:
https://academic.oup.com/mnras/article-abstract/494/1/17/5804816
https://arxiv.org/abs/2003.02783

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Semi-analytic modelling of the dynamics and outflows of stars with powerful winds.

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