Dr James Matthews: Publications

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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Shedding far-ultraviolet light on the donor star and evolutionary state of the neutron-star LMXB Swift J1858.6−0814

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 527:2 (2023) 2508-2522

Authors:

N Castro Segura, C Knigge, JH Matthews, FM Vincentelli, P Charles, KS Long, D Altamirano, DAH Buckley, D Modiano, MAP Torres, DJK Buisson, S Fijma, K Alabarta, N Degenaar, M Georganti, MC Baglio

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A disc wind model for blueshifts in quasar broad emission lines

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 526:3 (2023) 3967-3986

Authors:

James H Matthews, Jago Strong-Wright, Christian Knigge, Paul Hewett, Matthew J Temple, Knox S Long, Amy L Rankine, Matthew Stepney, Manda Banerji, Gordon T Richards

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A disc wind model for blueshifts in quasar broad emission lines

ArXiv 2309.14434 (2023)

Authors:

James H Matthews, Jago Strong-Wright, Christian Knigge, Paul Hewett, Matthew J Temple, Knox S Long, Amy L Rankine, Matthew Stepney, Manda Banerji, Gordon T Richards

Details from ArXiV

No redshift evolution in the rest-frame ultraviolet emission line properties of quasars from z = 1.5 to z = 4.0

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 524:4 (2023) 5497-5513

Authors:

Matthew Stepney, Manda Banerji, Paul C Hewett, Matthew J Temple, Amy L Rankine, James H Matthews, Gordon T Richards

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Dr James Matthews

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

Authors:

Shedding far-ultraviolet light on the donor star and evolutionary state of the neutron-star LMXB Swift J1858.6−0814

Authors:

A disc wind model for blueshifts in quasar broad emission lines

Authors:

A disc wind model for blueshifts in quasar broad emission lines

Authors:

No redshift evolution in the rest-frame ultraviolet emission line properties of quasars from z = 1.5 to z = 4.0

Authors:

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Dr James Matthews

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

Authors:

Shedding far-ultraviolet light on the donor star and evolutionary state of the neutron-star LMXB Swift J1858.6−0814

Authors:

A disc wind model for blueshifts in quasar broad emission lines

Authors:

A disc wind model for blueshifts in quasar broad emission lines

Authors:

No redshift evolution in the rest-frame ultraviolet emission line properties of quasars from z = 1.5 to z = 4.0

Authors: