activity
20092026
most citedDiscovery of extreme particle acceleration in the microquasar Cygnus X-3

207 citations · 406 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2026

Polarisation angle variability in tidal disruption events

A. Floris, I. Liodakis, K. I. I. Koljonen +9

Tidal disruption events (TDEs) occur when a star is disrupted by the tidal forces of a supermassive black hole, and these events produce bright multi-wavelength flares. Polarimetri…

astro-ph.HE2025

Polarimetric Diversity in Tidal Disruption Events: Comparative Study of Low-Polarised sources with AT2020mot

A. Floris, I. Liodakis, K. I. I. Koljonen +13

Tidal disruption events (TDEs) occur when a star is disrupted by the tidal forces of a supermassive black hole (SMBH), producing bright multi-wavelength flares. Among these events,…

astro-ph.HE2025

The peculiar hard state behaviour of the black hole X-ray binary Swift J1727.81613

A. K. Hughes, F. Carotenuto, T. D. Russell +37

Tracking the correlation between radio and X-ray luminosities during black hole X-ray binary outbursts is a key diagnostic of the coupling between accretion inflows (traced by X-ra…

astro-ph.HE2025★ 3 cited

Repeating flares, X-ray outbursts and delayed infrared emission: A comprehensive compilation of optical tidal disruption events

D. A. Langis, I. Liodakis, K. I. I. Koljonen +10

TDEs have been proposed as valuable laboratories for studying dormant black holes. However, progress in this field has been hampered by the limited number of observed events. In th…

astro-ph.HE2025

Jet break revealed in the transitional millisecond pulsar candidate 4FGL J0427.8-6704

K. I. I. Koljonen, M. Linares, J. C. A. Miller-Jones

Understanding the formation and properties of relativistic jets from accreting compact objects has far-reaching implications in astrophysics. Transitional millisecond pulsars (tMSP…

astro-ph.HE2023★ 19 cited

The origin of optical emission lines in the soft state of X-ray binary outbursts: the case of MAXI J1820+070

K. I. I. Koljonen, K. S. Long, J. H. Matthews +1

The optical emission line spectra of X-ray binaries (XRBs) are thought to be produced in an irradiated atmosphere, possibly the base of a wind, located above the outer accretion di…

astro-ph.HE2022★ 19 cited

Optical polarization from colliding stellar stream shocks in a tidal disruption event

I. Liodakis, K. I. I. Koljonen, D. Blinov +9

A tidal disruption event (TDE) occurs when a supermassive black hole rips apart a passing star. Part of the stellar material falls toward the black hole, forming an accretion disk…

astro-ph.HE2022★ 25 cited

Discovery of optical and infrared accretion disc wind signatures in the black hole candidate MAXI J1348-630

G. Panizo-Espinar, M. Armas Padilla, T. Muñoz-Darias +11

MAXI J1348-630 is a low mass X-ray binary discovered in 2019 during a bright outburst. During this event, the system sampled both hard and soft states following the standard evolut…

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.HE2011★ 37 cited

AGILE detection of Cygnus X-3 γ-ray active states during the period mid-2009/mid-2010

A. Bulgarelli, M. Tavani, A. W. Chen +70

Cygnus X-3 (Cyg X-3) is a well-known microquasar producing variable emission at all wavelengths. Cyg X-3 is a prominent X-ray binary producing relativistic jets, and studying its h…

astro-ph.HE2009★ 207 cited

Discovery of extreme particle acceleration in the microquasar Cygnus X-3

M. Tavani, A. Bulgarelli, G. Piano +67

The study of relativistic particle acceleration is a major topic of high-energy astrophysics. It is well known that massive black holes in active galaxies can release a substantial…

astro-ph.HE2009★ 72 cited

Orbital modulation of X-ray emission lines in Cygnus X-3

O. Vilhu, P. Hakala, D. C. Hannikainen +2

We address the problem where the X-ray emission lines are formed and investigate orbital dynamics using Chandra HETG observations, photoionizing calculations and numerical wind-par…