activity
20112023
most citedModelling the compact jet in MAXI J1836-194 with disc-driven shocks

24 citations · 97 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2023

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

F. M. Vincentelli, P. Casella, A. Borghese +23

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…

astro-ph.HE2023★ 24 cited

Matter ejections behind the highs and lows of the transitional millisecond pulsar PSR J1023+0038

M. C. Baglio, F. Coti Zelati, S. Campana +23

Transitional millisecond pulsars are an emerging class of sources that link low-mass X-ray binaries to millisecond radio pulsars in binary systems. These pulsars alternate between…

astro-ph.HE2023★ 7 cited

Short Timescale Evolution of the Polarized Radio Jet during V404 Cygni's 2015 Outburst

Andrew K. Hughes, Gregory R. Sivakoff, Christopher E. Macpherson +18

We present a high time resolution, multi-frequency linear polarization analysis of Very Large Array (VLA) radio observations during some of the brightest radio flaring (~1 Jy) acti…

astro-ph.HE2018★ 24 cited

Modelling the compact jet in MAXI J1836-194 with disc-driven shocks

Mathias Péault, Julien Malzac, Mickael Coriat +9

The black hole candidate MAXI J1836-194 was discovered in 2011 when it went into an outburst, and was the subject of numerous, quasi-simultaneous, multi-wavelength observations in…

astro-ph.HE2018★ 20 cited

Multiwavelength characterisation of the accreting millisecond X-ray pulsar and ultra-compact binary IGR J17062-6143

J. V. Hernandez Santisteban, V. Cuneo, N. Degenaar +8

IGR J17062-6143 is an ultra-compact X-ray binary (UCXB) with an orbital period of 37.96 min. It harbours a millisecond X-ray pulsar that is spinning at 163 Hz and and has continuou…

astro-ph.HE2011★ 22 cited

Jet trails and Mach cones: The interaction of microquasars with the ISM

Doosoo Yoon, Brian Morsony, Sebastian Heinz +4

A sub-set of microquasars exhibit high peculiar velocity with respect to the local standard of rest due to the kicks they receive when being born in supernovae. The interaction bet…