activity
20102026
most citedA wide and collimated radio jet in 3C 84 on the scale of a few hundred gravitational radii

135 citations · 541 across the 18 of their papers we have counts for

collaborators

16 papers

astro-ph.HE2026

Probing Physical Conditions in Classical and Symbiotic Novae with the Square Kilometre Array Observatory

Rocco Lico, Marcello Giroletti, Arnau Aguasca-Cabot +9

Cataclysmic variables and symbiotic stars are interacting binary systems in which a hot white dwarf (WD) orbits a companion main-sequence or red giant star, respectively. Accumulat…

astro-ph.HE2025

Fermi-LAT detections of novae V1723 Sco and V6598 Sgr

P. Fauverge, P. Jean, K. Sokolovsky +8

Context. Numerous classical novae have been observed to emit γ-rays (E > 100 MeV) detected by the Fermi-LAT. The prevailing hypothesis attributes this emission to the interaction o…

astro-ph.SR2025★ 4 cited

TCP J072226836220548: a new AM CVn type system with infrequent outbursts

Alexander Tarasenkov, Kirill Sokolovsky, Alexandr Dodin +11

We present the discovery of TCP J072226836220548, a new ultracompact binary system of the AM CVn type. This system was first identified displaying a mag outburst on 2…

astro-ph.HE2023★ 73 cited

A Shock Flash Breaking Out of a Dusty Red Supergiant

Gaici Li, Maokai Hu, Wenxiong Li +41

Shock breakout emission is light that arises when a shockwave, generated by core-collapse explosion of a massive star, passes through its outer envelope. Hitherto, the earliest det…

astro-ph.SR2020★ 48 cited

Gaia 18dvy: a new FUor in the Cygnus OB3 association

E. Szegedi-Elek, P. Ábrahám, L. Wyrzykowski +59

We present optical-infrared photometric and spectroscopic observations of Gaia18dvy, located in the Cygnus OB3 association at a distance of 1.88 kpc. The object was noted by the Ga…

astro-ph.GA2018★ 135 cited

A wide and collimated radio jet in 3C 84 on the scale of a few hundred gravitational radii

G. Giovannini, T. Savolainen, M. Orienti +22

Understanding the launching, acceleration, and collimation of jets powered by active galactic nuclei remains an outstanding problem in relativistic astrophysics. This is partly bec…