Qwind.jl

Computation of UV line-driven winds in AGNs
Author arnauqb
Popularity
2 Stars
Updated Last
3 Months Ago
Started In
June 2020

Qwind

CI codecov Documentation TagBot DOI

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!