Qwind
Qwind: Modelling UV line-driven winds originating from accretion discs
Qwind is a code that aims to simulate the launching and acceleration phase of line-driven winds in the context of AGN accretion discs. Refer to the paper for an explanation on the physics of the code.
Documentation
You can find the code documentation (with installation instructions) here
Citation
If you make use of the code, please cite the the paper. Here is a bibtex entry:
@article{qwind3,
author = {Quera-Bofarull, Arnau and Done, Chris and Lacey, Cedric G and Nomura, Mariko and Ohsuga, Ken},
title = "{qwind3: UV line-driven accretion disc wind models for AGN feedback}",
journal = {Monthly Notices of the Royal Astronomical Society},
volume = {518},
number = {2},
pages = {2693-2711},
year = {2022},
month = {11},
issn = {0035-8711},
doi = {10.1093/mnras/stac3171},
url = {https://doi.org/10.1093/mnras/stac3171},
eprint = {https://academic.oup.com/mnras/article-pdf/518/2/2693/47414762/stac3171.pdf},
}
Contributions
Contributions are very welcome!