How, where and when do cosmic rays reach ultrahigh energies?
(2023)
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
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
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
A disc wind model for blueshifts in quasar broad emission lines
ArXiv 2309.14434 (2023)