Dr James Matthews: Publications

SIROCCO: A Publicly Available Monte Carlo Ionization and Radiative Transfer Code for Astrophysical Outflows

ArXiv 2410.19908 (2024)

Authors:

James H Matthews, Knox S Long, Christian Knigge, Stuart A Sim, Edward J Parkinson, Nick Higginbottom, Samuel W Mangham, Nicolas Scepi, Austen Wallis, Henrietta A Hewitt, Amin Mosallanezhad

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A disc wind origin for the optical spectra of dwarf novae in outburst

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 532:1 (2024) 1199-1211

Authors:

Yusuke Tampo, Christian Knigge, Knox S Long, James H Matthews, Noel Castro Segura

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[O iii] emission in z ≈ 2 quasars with and without broad absorption lines

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 532:1 (2024) 424-437

Authors:

Matthew J Temple, Amy L Rankine, Manda Banerji, Joseph F Hennawi, Paul C Hewett, James H Matthews, Riccardo Nanni, Claudio Ricci, Gordon T Richards

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How, where and when do cosmic rays reach ultrahigh energies?

(2023)

Authors:

James H Matthews, Andrew M Taylor

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State-of-the-art simulations of line-driven accretion disc winds: realistic radiation hydrodynamics leads to weaker outflows

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 527:3 (2023) 9236-9249

Authors:

Nick Higginbottom, Nicolas Scepi, Christian Knigge, Knox S Long, James H Matthews, Stuart A Sim

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Dr James Matthews

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SIROCCO: A Publicly Available Monte Carlo Ionization and Radiative Transfer Code for Astrophysical Outflows

Authors:

A disc wind origin for the optical spectra of dwarf novae in outburst

Authors:

[O iii] emission in z ≈ 2 quasars with and without broad absorption lines

Authors:

How, where and when do cosmic rays reach ultrahigh energies?

Authors:

State-of-the-art simulations of line-driven accretion disc winds: realistic radiation hydrodynamics leads to weaker outflows

Authors:

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Dr James Matthews

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SIROCCO: A Publicly Available Monte Carlo Ionization and Radiative Transfer Code for Astrophysical Outflows

Authors:

A disc wind origin for the optical spectra of dwarf novae in outburst

Authors:

[O iii] emission in z ≈ 2 quasars with and without broad absorption lines

Authors:

How, where and when do cosmic rays reach ultrahigh energies?

Authors:

State-of-the-art simulations of line-driven accretion disc winds: realistic radiation hydrodynamics leads to weaker outflows

Authors: