activity
20132022
most citedAccretion disc atmospheres and winds in low-mass X-ray binaries

132 citations · 327 across the 6 of their papers we have counts for

collaborators

6 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.HE2021★ 4 cited

A search for signatures of interactions of X-ray binary outflows with their environments with ALMA

M. Díaz Trigo, D. Petry, E. Humphreys +2

We observed the X-ray binaries CirX-1, ScoX-1, GRS 1915+105, GX13+1, and CygX-1 with the Atacama Large Millimeter/submillimeter Array (ALMA). Unresolved continuum emission is found…

astro-ph.HE2018★ 26 cited

Modelling the disk atmosphere of the low mass X-ray binary EXO 0748-676

Ioanna Psaradaki, Elisa Costantini, Missagh Mehdipour +1

Low mass X-ray binaries exhibit ionized emission from an extended disk atmosphere that surrounds the accretion disk. However, its nature and geometry is still unclear. In this work…

astro-ph.HE2015★ 132 cited

Accretion disc atmospheres and winds in low-mass X-ray binaries

M. Díaz Trigo, L. Boirin

In the last decade, X-ray spectroscopy has enabled a wealth of discoveries of photoionised absorbers in X-ray binaries. Studies of such accretion disc atmospheres and winds are of…

astro-ph.HE2014★ 55 cited

XMM-Newton observations reveal the disappearance of the wind in 4U 1630-47

M. Díaz Trigo, S. Migliari, J. C. A. Miller-Jones +1

We report on XMM-Newton observations of the black hole X-ray binary 4U 1630-47 during its 2012-2013 outburst. The first five observations monitor the source as its luminosity incre…

astro-ph.HE2013★ 110 cited

Baryons in the relativistic jets of the stellar-mass black hole candidate 4U 1630-47

María Díaz Trigo, James C. A. Miller-Jones, Simone Migliari +2

Accreting black holes are known to power relativistic jets, both in stellar-mass binary systems and at the centres of galaxies. The power carried away by the jets, and hence the fe…