The black hole transient MAXI J1348–630: evolution of the compact and transient jets during its 2019/2020 outburst

F Carotenuto, S Corbel, E Tremou… - Monthly Notices of …, 2021 - academic.oup.com
We present the radio and X-ray monitoring campaign of the 2019/2020 outburst of MAXI
J1348–630, a new black hole X-ray binary (BH XRB) discovered in 2019 January. We …

Failed-transition outbursts in black hole low-mass X-ray binaries

K Alabarta, D Altamirano, M Méndez… - Monthly Notices of …, 2021 - academic.oup.com
Black hole low-mass X-ray binaries (BH LMXBs) evolve in a similar way during outburst.
Based on the X-ray spectrum and variability, this evolution can be divided into three …

Chasing the break: tracing the full evolution of a black hole X-ray binary jet with multiwavelength spectral modeling

C Echiburú-Trujillo, AJ Tetarenko… - The Astrophysical …, 2024 - iopscience.iop.org
Black hole (BH) X-ray binaries (XRBs) are ideal targets to study the connection between
accretion inflow and jet outflow. Here we present quasi-simultaneous, multiwavelength …

Doughnut strikes sandwich: the geometry of hot medium in accreting black hole X-ray binaries

J Poutanen, A Veledina, AA Zdziarski - Astronomy & Astrophysics, 2018 - aanda.org
We study the effects of the mutual interaction of hot plasma and cold medium in black hole
binaries in their hard spectral state. We consider a number of different geometries. In …

The black hole X-ray binary MAXI J1348–630 in quiescence

F Carotenuto, S Corbel… - Monthly Notices of the …, 2022 - academic.oup.com
The properties of the disc/jet coupling in quiescent black hole low mass X-ray binaries (BH
LMXBs) are still largely unknown. In this paper, we present the first quasi-simultaneous radio …

Sub-second infrared variability from the archetypal accreting neutron star 4U 1728− 34

FM Vincentelli, P Casella, A Borghese… - Monthly Notices of …, 2023 - academic.oup.com
We report on the first simultaneous high-time resolution X-ray and infrared (IR) observations
of a neutron star low mass X-ray binary in its hard state. We performed h of simultaneous …

Fast infrared variability from the black hole candidate MAXI J1535− 571 and tight constraints on the modelling

FM Vincentelli, P Casella, DM Russell… - Monthly Notices of …, 2021 - academic.oup.com
We present the results regarding the analysis of the fast X-ray/infrared (IR) variability of the
black hole transient MAXI J1535− 571. The data studied in this work consist of two strictly …

An optically thick disk wind in GRO J1655–40?

M Shidatsu, C Done, Y Ueda - The Astrophysical Journal, 2016 - iopscience.iop.org
We revisited the unusual wind in GRO J1655− 40, detected with Chandra in 2005 April,
using long-term Rossi X-ray Timing Explorer X-ray data and simultaneous optical/near …

Multiwavength observations of the black hole X-ray binary A0620-00 in quiescence

T Dinçer, CD Bailyn, JCA Miller-Jones… - The Astrophysical …, 2017 - iopscience.iop.org
We present results from simultaneous multiwavelength X-ray, radio, and optical/near-
infrared observations of the quiescent black hole X-ray binary A0620-00 performed in 2013 …

Lorentz factors of compact jets in black hole X-ray binaries

P Saikia, DM Russell, DM Bramich… - The Astrophysical …, 2019 - iopscience.iop.org
Compact, continuously launched jets in black hole X-ray binaries (BHXBs) produce radio to
optical/IR synchrotron emission. In most BHXBs, an IR excess (above the disk component) is …