activity
20182022
most citedThe thermal-radiative wind in the neutron star low mass X-ray binary GX 13+1

24 citations · 24 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2022

Accretion physics at high X-ray spectral resolution: New frontiers and game-changing science

P. Gandhi, T. Kawamuro, M. Díaz Trigo +14

Microcalorimeters have demonstrated success in delivering high spectral resolution, and have paved the path to revolutionary new science possibilities in the coming decade of X-ray…

astro-ph.HE202024 cited

The thermal-radiative wind in the neutron star low mass X-ray binary GX 13+1

Ryota Tomaru, Chris Done, Ken Ohsuga +2

We fit the observed high ionisation X-ray absorption lines in the neutron star binary GX13+1 with a full simulation of a thermal-radiative wind. This uses a radiation hydrodynamic…

astro-ph.HE2019

The thermal-radiative wind in low mass X-ray binary H 1743-322: II. iron line predictions from Monte Carlo radiation transfer

Ryota Tomaru, Chris Done, Ken Ohsuga +2

We show the best current simulations of the absorption and emission features predicted from thermal-radiative winds produced from X-ray illumination of the outer accretion disc in…

astro-ph.IM2019

The Voyage of Metals in the Universe from Cosmological to Planetary Scales: the need for a Very High-Resolution, High Throughput Soft X-ray Spectrometer

F. Nicastro, J. Kaastra, C. Argiroffi +27

Metals form an essential part of the Universe at all scales. Without metals we would not exist, and the Cosmos would look completely different. Metals are primarily born through nu…

astro-ph.HE2019

Thermally driven wind as the origin of warm absorbers in AGN

Misaki Mizumoto, Chris Done, Ryota Tomaru +1

Warm absorbers are present in many Active Galactic Nuclei (AGN), seen as mildly ionised gas outflowing with velocities of a few hundred to a few thousand kilometres per second. The…

astro-ph.HE2019

The thermal-radiative wind in low mass X-ray binary H 1743-322; Radiation hydrodynamic simulations

Ryota Tomaru, Chris Done, Ken Ohsuga +2

Blueshifted absorption lines are seen in high inclination black hole binary systems in their disc dominated states, showing these power an equatorial disc wind. While some contribu…