activity
19962023
most citedRadio / X-ray correlation in the low/hard state of GX 339--4

450 citations · 7.7k across the 126 of their papers we have counts for

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Showing 2021Show all

6 papers · 1 filter

astro-ph.GA2021★ 1 cited

Pilot study and early results of the Cosmic Filaments and Magnetism Survey with Nenufar: the Coma cluster field

Bonnassieux Etienne, Evangelia Tremou, Julien N. Girard +9

NenuFAR, the New Extension in Nancay Upgrading LOFAR, is currently in its early science phase. It is in this context that the Cosmic Filaments and Magnetism Pilot Survey is observi…

astro-ph.SR2021★ 1 cited

Observations of shock propagation through turbulent plasma in the solar corona

Eoin P. Carley, Baptiste Cecconi, Hamish A. Reid +14

Eruptive activity in the solar corona can often lead to the propagation of shock waves. In the radio domain the primary signature of such shocks are type II radio bursts, observed…

astro-ph.HE2021★ 29 cited

The hybrid radio/X-ray correlation of the black hole transient MAXI J1348-630

F. Carotenuto, S. Corbel, E. Tremou +8

Black hole low mass X-ray binaries in their hard spectral state are found to display two different correlations between the radio emission from the compact jets and the X-ray emiss…

astro-ph.HE2021★ 4 cited

Strong low-frequency radio flaring from Cygnus X-3 observed with LOFAR

J. W. Broderick, T. D. Russell, R. P. Fender +12

We present Low-Frequency Array (LOFAR) 143.5-MHz radio observations of flaring activity during 2019 May from the X-ray binary Cygnus X-3. Similar to radio observations of previous…

astro-ph.HE2021★ 80 cited

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 +14

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 (XRB) discovered in 2019 January. We observed MAXI J13…

astro-ph.HE2021★ 1 cited

Expected disk wind properties evolution along an X-ray Binary outburst

P. -O. Petrucci, S. Bianchi, G. Ponti +12

Blueshifted X-ray absorption lines (preferentially from Fe XXV and Fe XXVI present in the 6-8 keV range) indicating the presence of massive hot disk winds in Black Hole (BH) X-ray…