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20162026
most citedRapid compact jet quenching in the Galactic black hole candidate X-ray binary MAXI J1535-571

49 citations · 350 across the 20 of their papers we have counts for

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Showing 2020 · astro-ph.HEShow all

7 papers · 2 filters

astro-ph.HE2020★ 49 cited

Rapid compact jet quenching in the Galactic black hole candidate X-ray binary MAXI J1535-571

T. D. Russell, M. Lucchini, A. J. Tetarenko +23

We present results from six epochs of quasi-simultaneous radio, (sub-)millimetre, infrared, optical, and X-ray observations of the black hole X-ray binary MAXI~J1535571. These o…

astro-ph.HE2020★ 14 cited

Soft X-ray emission lines in the X-ray binary Swift J1858.6-0814 observed with XMM-Newton-RGS: disc atmosphere or wind?

D. J. K. Buisson, D. Altamirano, M. Díaz Trigo +11

We find soft X-ray emission lines from the X-ray binary Swift J1858.6-0814 in data from XMM-Newton-RGS: N VII, O VII and O VIII, as well as notable residuals short of a detection a…

astro-ph.HE2020

Detection of two bright radio bursts from magnetar SGR 1935+2154

F. Kirsten, M. Snelders, M. Jenkins +5

Fast radio bursts (FRBs) are millisecond-duration, bright radio signals (fluence ) emitted from extragalactic sources of unknown physical origin. The re…

astro-ph.HE2020★ 22 cited

The variable radio counterpart of Swift J1858.6-0814

J. van den Eijnden, N. Degenaar, T. D. Russell +18

Swift J1858.6-0814 is a transient neutron star X-ray binary discovered in October 2018. Multi-wavelength follow-up observations across the electromagnetic spectrum revealed many in…

astro-ph.HE2020

The Changing-look Optical Wind of the Flaring X-ray Transient Swift J1858.6-0814

T. Muñoz-Darias, M. Armas Padilla, F. Jiménez-Ibarra +15

We present the discovery of an optical accretion disk wind in the X-ray transient Swift J1858.6-0814. Our 90-spectrum data set, taken with the 10.4m GTC telescope over 8 different…

astro-ph.HE2020★ 15 cited

A strongly changing accretion morphology during the outburst decay of the neutron star X-ray binary 4U 1608-52

J. van den Eijnden, N. Degenaar, R. M. Ludlam +7

It is commonly assumed that the properties and geometry of the accretion flow in transient low-mass X-ray binaries (LMXBs) significantly change when the X-ray luminosity decays bel…