activity
20162026
most citedNine-hour X-ray quasi-periodic eruptions from a low-mass black hole galactic nucleus

295 citations · 565 across the 42 of their papers we have counts for

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5 papers · 1 filter

astro-ph.SR2026

SXP 31.0 -- the 2025 near-Eddington double X-ray outburst after 26 years of quiescence

Malcolm J. Coe, Thomas M. Gaudin, Itumeleng M. Monageng +5

SXP 31.0 is an X-ray source in the Small Magellanic Cloud (SMC) that was first identified as a Be X-ray Binary (BeXRB) system when it went into X-ray outbusrst in 1998. It is now k…

astro-ph.SR2025

An extremely fast fading population II dwarf nova candidate: caught spectroscopically on the rise

Natasha Van Bemmel, Jielai Zhang, Jeff Cooke +14

We present AT2022kak, a rapidly evolving optical transient discovered by the KiloNova and Transients Program (KNTraP). This interesting burst exhibited extremely fast evolution, wi…

astro-ph.SR2022★ 20 cited

Three new high-mass X-ray binaries in the Large Magellanic Cloud

F. Haberl, C. Maitra, G. Vasilopoulos +4

The Magellanic Clouds host a large population of high-mass X-ray binary (HMXB) systems, but although the Large Magellanic Cloud (LMC) is an order of magnitude more massive than the…

astro-ph.SR2021★ 1 cited

The VLT-FLAMES survey of massive stars. NGC2004#115: A triple system hosting a possible short period B+BH binary

D. J. Lennon, P. L. Dufton, J. I. Villaseñor +5

The star NGC2004#115 in the LMC, originally classified as an (SB1) Be spectroscopic binary, bears some morphological resemblance to the Galactic systems LB-1 and HR 6819, both of w…

astro-ph.SR2020★ 7 cited

Optical and X-ray study of the peculiar high mass X-ray binary XMMU J010331.7-730144

Itumeleng M. Monageng, Malcolm J. Coe, David A. H. Buckley +6

For a long time XMMU J010331.7-730144 was proposed as a high-mass X-ray binary candidate based on its X-ray properties, however, its optical behaviour was unclear - in particular p…