activity
19942022
most citedJet stability and the generation of superluminal and stationary components

144 citations · 1.2k across the 57 of their papers we have counts for

collaborators

57 papers

astro-ph.HE2022★ 2 cited

Magnetization of Relativistic Current-Carrying Jets with Radial Velocity Shear

Dominika Ł. Król, Łukasz Stawarz, Mitchell C. Begelman +3

Astrophysical jets, launched from the immediate vicinity of accreting black holes, carry away large amounts of power in a form of bulk kinetic energy of jet particles and electroma…

astro-ph.GA2021★ 59 cited

Reading M87's DNA: A Double Helix revealing a large scale Helical Magnetic Field

Alice Pasetto, Carlos Carrasco-Gonzalez, Jose L. Gomez +7

We present unprecedented high fidelity radio images of the M87 jet. We analyzed Jansky Very Large Array (VLA) broadband, full polarization, radio data from 4 to 18 GHz. The observa…

astro-ph.HE2021★ 21 cited

Long-term FRII jet evolution in dense environments

Manel Perucho, José María Martí, Vicent Quilis

We present long-term numerical three-dimensional simulations of a relativistic outflow propagating through a galactic ambient medium and environment, up to distances ~kpc…

astro-ph.SR2021★ 6 cited

The symbiotic binary ZZ CMi: intranight variability and suggested outbursting nature

R. K. Zamanov, K. A. Stoyanov, A. Kostov +9

We present photometric and spectral observations of the symbiotic star ZZ CMi. We detect intranight variability - flickering and smooth variations in U band. The amplitude of the f…

astro-ph.SR2020

Intra-night flickering of RS Ophiuchi: III. Modes of quasi-periods in the minute scale and their evolution

Ts. B. Georgiev, R. K. Zamanov, S. Boeva +7

We study the photometric behavior of the recurrent nova RS Oph by 58 monitoring light curves (LCs), taken by 5 telescopes. All LCs show repeating time structures with some quasi-pe…

astro-ph.SR2018

Intra-night flickering of RS Ophiuchi: I. Sizes and cumulative energies of time structures

Ts. B. Georgiev, R. K. Zamanov, S. Boeva +7

We analyzed 29 pairs of time series in B and V bands of the recurrent nova RS Oph. The observations were carried out in 2008-2017 with duration 0.6 - 3.6 hours, with time resolutio…