activity
20002026
most citedFilaments, Bubbles, and Weak Shocks in the Gaseous Atmosphere of M87

324 citations · 2.4k across the 32 of their papers we have counts for

collaborators

32 papers

astro-ph.GA2026

Odd Radio Circles Modeled by Shock-Bubble Interactions

Yiting Wang, Sebastian Heinz

The physical nature and origins of the newly discovered class of Odd Radio Circles (ORCs) remain unclear. We investigate a model whereby ORCs are synchrotron-emitting vortex rings…

astro-ph.HE2026

The Self-Limiting Nature of Jet-Modulated Thermal Conduction in Cool Core Clusters

Jennifer Stafford, Sebastian Heinz, Mateusz Ruszkowski +2

Conduction as a mechanism for explaining the disrupted cooling-flow in galaxy clusters has been mostly discounted, as the process is inefficient at transporting heat all the way fr…

astro-ph.HE2024★ 13 cited

Astroparticles from X-ray Binary Coronae

Ke Fang, Francis Halzen, Sebastian Heinz +1

The recent observation of high-energy neutrinos from the Galactic plane implies an abundant population of hadronic cosmic-ray sources in the Milky Way. We explore the role of the c…

astro-ph.HE2024

The cause of the difference in the propagation distances between compact and transient jets in black-hole X-ray binaries

Andrzej A. Zdziarski, Sebastian Heinz

Accreting black-hole binaries change their properties during evolution, passing through two main luminous states, dominated by either hard or soft X-rays. In the hard state, steady…

astro-ph.HE2023★ 23 cited

Chasing the break: Tracing the full evolution of a black hole X-ray binary jet with multi-wavelength spectral modeling

Constanza Echiburú-Trujillo, Alexandra J. Tetarenko, Daryl Haggard +35

Black hole X-ray binaries (BH XRBs) are ideal targets to study the connection between accretion inflow and jet outflow. Here we present quasi-simultaneous, multi-wavelength observa…

astro-ph.HE2020★ 17 cited

The Origins of X-ray Line Emissions in Circinus~X-1 at Very Low X-ray Flux

N. S. Schulz, T. E. Kallman, S. Heinz +3

Accretion conditions and morphologies of X-ray transients containing neutron stars are still poorly understood. Circinus X-1 is an enigmatic case where we observe X-ray flux change…