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The complex evolution of the X-ray binary transient MAXI J1807+132 along the decay of its discovery outburst
F. Jiménez-Ibarra, T. Muñoz-Darias, M. Armas Padilla +6
MAXI J1807+132 is an X-ray transient discovered during the decay of an outburst in 2017. We present optical and X-ray monitoring of the source over more than 125 days, from outburs…
The radio/X-ray correlation in X-ray binaries - Insights from a hard X-ray perspective
Karri I. I. Koljonen, David M. Russell
The radio/X-ray correlation is one of the most important pieces of observational evidence of the disk-jet connection in accreting compact objects. However, a growing number of X-ra…
The Curious Case of Swift J1753.5-0127: A Black Hole Low-mass X-ray Binary Analogue to Z Cam Type Dwarf Novae
A. W. Shaw, B. E. Tetarenko, G. Dubus +5
Swift J1753.5-0127 (J1753) is a candidate black hole low-mass X-ray binary (BH-LMXB) that was discovered in outburst in May 2005. It remained in outburst for years, exhibi…
Tracking the variable jets of V404 Cygni during its 2015 outburst
A. J. Tetarenko, G. R. Sivakoff, J. C. A. Miller-Jones +14
We present multi-frequency monitoring observations of the black hole X-ray binary V404 Cygni throughout its June 2015 outburst. Our data set includes radio and mm/sub-mm photometry…
Swift UVOT observations of the 2015 outburst of V404 Cygni
S. R. Oates, S. Motta, A. P. Beardmore +10
The black-hole binary, V404 Cygni, went into outburst in June 2015, after 26 years of X-ray quiescence. We observed the outburst with the Neil Gehrels Swift observatory. We present…
A jet model for the fast IR variability of the black hole X-ray binary GX 339-4
Julien Malzac, Maithili Kalamkar, Federico Vincentelli +16
Using the simultaneous Infra-Red (IR) and X-ray light curves obtained by Kalamkar et al. (2016), we perform a Fourier analysis of the IR/X-ray timing correlations of the black hole…