activity
20162026
most citedDiscovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds

169 citations · 529 across the 36 of their papers we have counts for

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Showing 2023Show all

14 papers · 1 filter

astro-ph.HE2023★ 3 cited

Unveiling the origin of the optical/UV emission from the Galactic ULX Swift J0243.6+6124 during its 2017-2018 giant outburst

J. Alfonso-Garzón, J. van den Eijnden, N. P. M. Kuin +8

From late September 2017 to February 2018, the Be X-ray binary (BeXB) Swift J0243.6+6124 underwent an unprecedently bright giant outburst. The reported X-ray luminosities were so h…

astro-ph.HE2023★ 6 cited

Evidence for a dynamic corona in the short-term time lags of black hole X-ray binary MAXI J1820+070

Niek Bollemeijer, Phil Uttley, Arkadip Basak +19

In X-ray observations of hard state black hole X-ray binaries, rapid variations in accretion disc and coronal power-law emission are correlated and show Fourier-frequency-dependent…

astro-ph.HE2023

SAX J1810.8-2609: An Outbursting Neutron Star X-ray Binary with Persistent Spatially Coincident Radio Emission

A. K. Hughes, G. R. Sivakoff, J. van den Eijnden +3

Here we report on joint X-ray and radio monitoring of the neutron star low-mass X-ray binary SAX J1810.8-2609. Our monitoring covered the entirety of its ~5 month outburst in 2021,…

astro-ph.HE2023

The nature of very-faint X-ray binaries: Near-infrared spectroscopy of 1RXH J173523.7354013 reveals a giant companion

A. W. Shaw, N. Degenaar, T. J. Maccarone +3

Very-faint X-ray binaries (VFXBs) are a sub-class of black holes and neutron stars in binaries that appear to be accreting at a very low rate. In addition to providing interesting…

astro-ph.HE2023★ 1 cited

The High Energy X-ray Probe (HEX-P): A New Window into Neutron Star Accretion

R. M. Ludlam, C. Malacaria, E. Sokolova-Lapa +15

Accreting neutron stars (NSs) represent a unique laboratory for probing the physics of accretion in the presence of strong magnetic fields ( G). Additionally, the ma…

astro-ph.HE2023★ 1 cited

VLA monitoring of LS V +44 17 reveals scatter in the X-ray--radio correlation of Be/X-ray binaries

J. van den Eijnden, A. Rouco Escorial, J. Alfonso-Garzón +8

LS V +44 17 is a persistent Be/X-ray binary (BeXRB) that displayed a bright, double-peaked period of X-ray activity in late 2022/early 2023. We present a radio monitoring campaign…

astro-ph.HE2023★ 1 cited

X-ray and Radio Monitoring of the Neutron Star Low Mass X-ray Binary 1A 1744-361: Quasi Periodic Oscillations, Transient Ejections, and a Disk Atmosphere

Mason Ng, Andrew K. Hughes, Jeroen Homan +19

We report on X-ray (NICER/NuSTAR/MAXI/Swift) and radio (MeerKAT) timing and spectroscopic analysis from a three-month monitoring campaign in 2022 of a high-intensity outburst of th…

astro-ph.HE2023

The first mm detection of a neutron star high-mass X-ray binary

J. van den Eijnden, L. Sidoli, M. Diaz Trigo +9

Neutron stars accreting from OB supergiants are often divided between persistently and transiently accreting systems, called Supergiant X-ray Binaries (SgXBs) and Supergiant Fast X…

astro-ph.HE2023★ 16 cited

The accretion/ejection link in the neutron star X-ray binary 4U 1820-30 I: A boundary layer-jet coupling?

A. Marino, T. D. Russell, M. Del Santo +16

The accretion flow / jet correlation in neutron star (NS) low-mass X-ray binaries (LMXBs) is far less understood when compared to black hole (BH) LMXBs. In this paper we will prese…

astro-ph.HE2023★ 1 cited

Accretion spin-up and a strong magnetic field in the slow-spinning Be X-ray binary MAXI J0655-013

Sean N. Pike, Mutsumi Sugizaki, Jakob van den Eijnden +8

We present MAXI and NuSTAR observations of the Be X-ray binary, MAXI J0655-013, in outburst. NuSTAR observed the source once early in the outburst, when spectral analysis yields a…

astro-ph.HE2023★ 13 cited

Expectations for Fast Radio Bursts in Neutron Star-Massive Star binaries

Kaustubh Rajwade, Jakob van den Eijnden

Recent observations of a small sample of repeating Fast Radio Bursts (FRBs) have revealed a periodicity in their bursting activity that may be suggestive of a binary origin for the…

astro-ph.HE2023★ 38 cited

A shared accretion instability for black holes and neutron stars

F. M. Vincentelli, J. Neilsen, A. J. Tetarenko +20

Accretion disks around compact objects are expected to enter an unstable phase at high luminosity. One instability may occur when the radiation pressure generated by accretion modi…

astro-ph.HE2023★ 8 cited

The 2019 outburst of AMXP SAX J1808.4-3658 and radio follow up of MAXI J0911-655 and XTE J1701-462

K. V. S. Gasealahwe, I. M. Monageng, R. P. Fender +14

We present radio coverage of the 2019 outburst of the accreting millisecond X-ray pulsar SAX J1808.4-3658, obtained with MeerKAT. We compare these data to contemporaneous X-ray and…

astro-ph.HE2023★ 10 cited

The Link Between Neutron Star X-ray Binaries and Spider Pulsars

Amy H. Knight, Adam Ingram, Jakob van den Eijnden +3

The discovery of transitional millisecond pulsars (tMSPs) provided conclusive proof that neutron star (NS) low-mass X-ray binaries (LMXBs) comprise part of the evolutionary pathway…