activity
20102026
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 9.7k across the 184 of their papers we have counts for

collaborators
Showing 2022Show all

15 papers · 1 filter

astro-ph.HE2022★ 82 cited

The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole

Dheeraj R. Pasham, Matteo Lucchini, Tanmoy Laskar +63

A black hole can launch a powerful relativistic jet after it tidally disrupts a star. If this jet fortuitously aligns with our line of sight, the overall brightness is Doppler boos…

astro-ph.GA2022★ 32 cited

Explaining the moderate UV/X-ray correlation in AGN

Christos Panagiotou, Erin Kara, Michal Dovčiak

The UV/optical and X-ray variability of active galactic nuclei (AGN) have long been expected to be well correlated as a result of the X-ray illumination of the accretion disk. Rece…

astro-ph.HE2022★ 25 cited

TPHO: a time-dependent photoionisation model for AGN outflows

Daniele Rogantini, Missagh Mehdipour, Jelle Kaastra +3

Outflows in active galactic nuclei (AGN) are considered a promising candidate for driving AGN feedback at large scales. However, without information on the density of these outflow…

astro-ph.HE2022★ 20 cited

X-ray Reverberation Mapping of Ark 564 using Gaussian Process Regression

Collin D. Lewin, Erin Kara, Daniel R. Wilkins +15

Ark 564 is an extreme high-Eddington Narrow-line Seyfert 1 galaxy, known for being one of the brightest, most rapidly variable soft X-ray AGN, and for having one of the lowest temp…

astro-ph.SR2022★ 19 cited

A dense star in a 51-minute orbital period eclipsing binary

Kevin B. Burdge, Kareem El-Badry, Thomas R. Marsh +24

In over a thousand known cataclysmic variables (CVs), where a white dwarf is accreting from a hydrogen-rich star, only a dozen have orbital periods below 75 minutes. One way to ach…

astro-ph.HE2022★ 9 cited

The long stare at Hercules X-1 -- I. Emission lines from the outer disk, the magnetosphere boundary and the accretion curtain

P. Kosec, E. Kara, A. C. Fabian +11

Hercules X-1 is a nearly edge-on accreting X-ray pulsar with a warped accretion disk, precessing with a period of about 35 days. The disk precession allows for unique and changing…

astro-ph.GA2022★ 50 cited

The Host Galaxy and Rapidly Evolving Broad-line Region in the Changing-look Active Galactic Nucleus 1ES 1927+654

Ruancun Li, Luis C. Ho, Claudio Ricci +4

Changing-look active galactic nuclei (AGNs) present an important laboratory to understand the origin and physical properties of the broad-line region (BLR). We investigate follow-u…

astro-ph.GA2022★ 28 cited

A physical model for the UV/optical power spectra of AGN

Christos Panagiotou, Iossif Papadakis, Erin Kara +2

The UV/optical variability of AGN has long been thought to be driven by the X-ray illumination of the accretion disk. However, recent multi-wavelength campaigns of nearby Seyfert g…

astro-ph.HE2022★ 44 cited

Evolution of a Relativistic Outflow and X-ray Corona in the Extreme Changing-Look AGN 1ES 1927+654

Megan Masterson, Erin Kara, Claudio Ricci +8

1ES 1927+654 is a paradigm-defying AGN and one of the most peculiar X-ray nuclear transients. In early 2018, this well-known AGN underwent a changing-look event, in which broad opt…

astro-ph.HE2022★ 18 cited

Black holes: Timing and spectral properties and evolution

Emrah Kalemci, Erin Kara, John A. Tomsick

We review the timing and spectral evolution of black hole X-ray binary systems, with emphasis on the current accretion-ejection paradigm. When in outburst, stellar mass black hole…

astro-ph.HE2022★ 18 cited

SRGA J181414.6-225604: A new Galactic symbiotic X-ray binary outburst triggered by an intense mass loss episode of a heavily obscured Mira variable

Kishalay De, Ilya Mereminskiy, Roberto Soria +24

We present the discovery and multi-wavelength characterization of SRGA J181414.6-225604, a Galactic hard X-ray transient discovered during the ongoing SRG/ART-XC sky survey. Using…

astro-ph.HE2022★ 24 cited

A 62-minute orbital period black widow binary in a wide hierarchical triple

Kevin B. Burdge, Thomas R. Marsh, Jim Fuller +30

Over a dozen millisecond pulsars are ablating low-mass companions in close binary systems. In the original "black widow", the 8-hour orbital period eclipsing pulsar PSR J1959+2048…

astro-ph.HE2022★ 62 cited

The NICER "Reverberation Machine": A Systematic Study of Time Lags in Black Hole X-Ray Binaries

Jingyi Wang, Erin Kara, Matteo Lucchini +12

We perform the first systematic search of all NICER archival observations of black hole (and candidate) low-mass X-ray binaries for signatures of reverberation. Reverberation lags…

astro-ph.HE2022★ 17 cited

Ejection-accretion connection in NLS1 AGN 1H 1934-063

Yerong Xu, Ciro Pinto, Erin Kara +7

Accretion and ejection of matter in active galactic nuclei (AGN) are tightly connected phenomena and represent fundamental mechanisms regulating the growth of the central supermass…

astro-ph.HE2022★ 70 cited

The complex time and energy evolution of quasi-periodic eruptions in eRO-QPE1

R. Arcodia, G. Miniutti, G. Ponti +8

Quasi-periodic eruptions (QPEs) are recurrent X-ray bursts found so far in the nuclei of low-mass galaxies. Their trigger mechanism is still unknown, but recent models involving on…