activity
20132026
most citedThe Milky Way's Supermassive Black Hole: How good a case is it? A Challenge for Astrophysics & Philosophy of Science

129 citations · 1.7k across the 78 of their papers we have counts for

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29 papers · 1 filter

astro-ph.HE2026

Low-angular-momentum accretion shocks can power weak-to-moderate X-ray flares from SgrA*

Samik Mitra, Bożena Czerny, Michal Zajaček +1

X-ray flares from Sgr~A* span broad ranges in duration, fluence, and luminosity, but their origin remains unsettled. We test whether standing shocks in low-angular-momentum magneti…

astro-ph.HE2026

What is the reason for the lack of cool evolved stars near the center of the Galaxy?

Petr Kurfürst, Michal Zajaček, Norbert Werner +2

The observed deficit of bright late-type giants in the central parsec of the Milky Way remains an open problem. We investigate whether repeated passages of red giants (RGs) through…

astro-ph.HE2026

Observations of X-ray quasi-periodic eruptions

Thomas Wevers, Joheen Chakraborty, Erwan Quintin +2

Quasi-periodic eruptions (QPEs) are a novel class of repeating nuclear transients, discovered exclusively in the X-ray band to date. Since their initial discovery in 2019, the QPE…

astro-ph.HE2026

Tidal disruption of a low-mass star in an active galactic nucleus as the origin of the PS16dtm outburst

Marzena Śniegowska, Bożena Czerny, Michal Zajaček +7

The event PS16dtm, which occured in the center of the Narrow Line Seyfert 1 (NLS1) galaxy SDSS J015804.75-005221.8 (z = 0.080440), is one of the few candidates for a tidal disrupti…

astro-ph.HE2026

Evolution of Quasi-Periodic Eruptions in the post-TDE Accretion Disk Perturbed by an Orbiting Star

Martin Mondek, Michal Zajaček, Henry Best +3

Quasi-periodic eruptions (QPEs) are a recently discovered class of highly variable X-ray bursts originating in galactic nuclei. These high-amplitude bursts exhibit periodicity rang…

astro-ph.HE2025★ 1 cited

Non-orbital particle trapping in binary black holes through dynamic stability

Ali Kurmus, Michal Zajacek, Greg Kestin +1

We present an interdisciplinary comparison between binary black hole systems and Radio Frequency (RF) Paul Traps, modeling the gravitational binary system as a rotating saddle near…

astro-ph.HE2024

Repeated Partial Tidal Disruptions and Quasi-Periodic Eruptions in SwJ023017.0+283603

Dheeraj Pasham, Eric Coughlin, Chris Nixon +5

SwJ023017.0+283603 (SwJ0230) exhibited soft X-ray (0.3-1.0 keV) eruptions recurring roughly every 22 days. We present results from an extended monitoring campaign of SwJ0230 using…

astro-ph.HE2024★ 19 cited

Repeating Nuclear Transients as Candidate Electromagnetic Counterparts of LISA Extreme Mass Ratio Inspirals

Shubham Kejriwal, Vojtech Witzany, Michal Zajacek +2

Extreme-mass-ratio inspirals (EMRIs) are one of the primary targets for the recently adopted millihertz gravitational-wave (GW) observatory LISA. Some previous studies have argued…

astro-ph.HE2024★ 30 cited

A Case for a Binary Black Hole System Revealed via Quasi-Periodic Outflows

Dheeraj R. Pasham, Francesco Tombesi, Petra Sukova +33

Binaries containing a compact object orbiting a supermassive black hole are thought to be precursors of gravitational wave events, but their identification has been extremely chall…

astro-ph.HE2024★ 22 cited

Alive but Barely Kicking: News from 3+ years of Swift and XMM-Newton X-ray Monitoring of Quasi-Periodic Eruptions from eRO-QPE1

Dheeraj R. Pasham, Eric R. Coughlin, Michal Zajacek +11

Quasi-periodic Eruptions (QPEs) represent a novel class of extragalactic X-ray transients that are known to repeat at roughly regular intervals of a few hours to days. Their underl…

astro-ph.HE2024★ 32 cited

Lense-Thirring Precession after a Supermassive Black Hole Disrupts a Star

Dheeraj R. Pasham, Michal Zajacek, C. J. Nixon +8

An accretion disk formed around a supermassive black hole (SMBH) after it disrupts a star is expected to be initially misaligned with respect to the black hole's equatorial plane.…

astro-ph.HE2023

MAD UFOs: Magnetically Arrested Discs with persistent Ultra-Fast Outflows

Petra Suková, Michal Zajaček, Vladimír Karas

General-relativistic magneto-hydrodynamical (GRMHD) simulations of accreting black holes suggest that the accretion flows form toroidal structures embedded in a large scale compone…

astro-ph.HE2023★ 64 cited

X-ray eruptions every 22 days from the nucleus of a nearby galaxy

Muryel Guolo, Dheeraj R. Pasham, Michal Zajaček +15

Galactic nuclei showing recurrent phases of activity and quiescence have recently been discovered, with recurrence times as short as a few hours to a day -- known as quasi-periodic…

astro-ph.HE2023★ 42 cited

Precession-induced Variability in AGN Jets and OJ 287

Silke Britzen, Michal Zajaček, Gopal-Krishna +5

The combined study of the flaring of Active Galactic Nuclei (AGN) at radio wavelengths and pc-scale jet kinematics with Very Long Baseline Interferometry (VLBI) has led to the view…

astro-ph.HE2023★ 2 cited

Science with a small two-band UV-photometry mission III: Active Galactic Nuclei and nuclear transients

M. Zajaček, B. Czerny, V. K. Jaiswal +14

In this review (the third in the series focused on a small two-band UV-photometry mission), we assess possibilities for a small UV two-band photometry mission in studying accreting…

astro-ph.HE2023

Science with a small two-band UV-photometry mission I: Mission description and follow-up observations of stellar transients

N. Werner, J. Řípa, C. Thöne +33

This is the first in a collection of three papers introducing the science with an ultra-violet (UV) space telescope on an approximately 130~kg small satellite with a moderately fas…

astro-ph.HE2023★ 5 cited

Spectral Energy Distribution profiles from AGN accretion disc in multi-gap setup

Marcel Štolc, Michal Zajaček, Bożena Czerny +1

Spectral Energy Distribution (SED) of the broad-band continuum emission from black-hole accretion discs can serve as a tool to measure parameters of the central body and constrain…

astro-ph.HE2023★ 22 cited

Radio jet precession in M81*

S. D. von Fellenberg, M. Janssen, J. Davelaar +5

We report four novel position angle measurements of the core region of M81* at 5GHz and 8GHz, which confirm the presence of sinusoidal jet precession of the M81 jet region as sugge…

astro-ph.HE2022

Non-thermal emission from fall-back clouds in the Broad-Line Region of Active Galactic Nuclei

Ana Laura Müller, Mohammad-Hassan Naddaf, Michal Zajaček +3

The spectra of active galactic nuclei exhibit broad-emission lines that presumably originate in the Broad-Line Region (BLR) with gaseous-dusty clouds in a predominantly Keplerian m…

astro-ph.HE2021★ 8 cited

Electromagnetic signatures of strong-field gravity from accreting black holes

Vladimir Karas, Michal Zajacek, Devaky Kunneriath +1

Observations of galactic nuclei help us to test General Relativity. Whereas the No-hair Theorem states that classical, isolated black holes eventually settle to a stationary state…

astro-ph.HE2021★ 96 cited

Stellar transits across a magnetized accretion torus as a mechanism for plasmoid ejection

Petra Suková, Michal Zajaček, Vojtěch Witzany +1

The close neighbourhood of a supermassive black hole contains not only the accreting gas and dust but also stellar-sized objects, such as late-type and early-type stars and compact…

astro-ph.HE2020★ 24 cited

Depletion of bright red giants in the Galactic center during its active phases

Michal Zajaček, Anabella Araudo, Vladimír Karas +2

Observations in the near-infrared domain showed the presence of the flat core of bright late-type stars inside from the Galactic center supermassive black hole…

astro-ph.HE2019★ 40 cited

Current and future applications of Reverberation-mapped quasars in Cosmology

Swayamtrupta Panda, Mary Loli Martínez-Aldama, Michal Zajaček

Reverberation mapping technique is an important milestone in AGN demographics, kinematics and the structure of the Broad Line Region (BLR) based on the time-delay response between…

astro-ph.HE2019

Super-Massive Black Hole mass estimation from bright flares

Vladimir Karas, Michal Bursa, Michal Dovciak +4

Super-Massive Black Holes reside in galactic nuclei, where they exhibit episodic bright flares due to accretion events. Taking into account relativistic effects, namely, the boosti…