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20242026
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astro-ph.HE2026

Thermal or Non-thermal? Diffuse emission in the infall region of stacked galaxy groups

E. Bulbul, X. Zhang, Z. Ding +16

The authors stack eROSITA X‑ray data for 827 low‑mass galaxy groups to detect faint diffuse emission out to ~2 R200, measuring temperature, density, and metal abundance in the infa…

astro-ph.HE2026

Idealized Global Models of Accretion Disks with Strong Toroidal Magnetic Fields

Minghao Guo, Eliot Quataert, Jonathan Squire +2

We present global magnetohydrodynamic (MHD) simulations of idealized accretion disks with a strong toroidal magnetic field using an equation of state that fixes the gas thermal sca…

astro-ph.HE2026

Resolving the (Debate About) Nozzle Shocks in Tidal Disruption Events

Zachary L. Andalman, Eliot Quataert, Eric R. Coughlin +1

When a star passes within the Roche limit of a supermassive black hole (SMBH), it is pulled apart by the BH's tidal field in a tidal disruption event (TDE). The resulting flare is…

astro-ph.HE2026

Self-Limited Accretion onto Embedded Binaries in a Uniform Medium

Marcus DuPont, Eliot Quataert

We study accretion from a uniform gas at rest onto equal-mass binaries -- the binary Bondi problem -- as a function of adiabatic index~ and compactness , where…

astro-ph.HE2026

X-ray Transmission Through Photoionized Gas with Moderate Thomson Optical Depth

Taya Govreen-Segal, Ehud Nakar, Eliot Quataert

We model the absorption of X-rays by gas obscuring the source and photoionized by it. We consider a broad range of column densities, including both Thomson-thin and Thomson-thick m…

astro-ph.HE2026

AT2018cow Powered by a Shock in Aspherical Circumstellar Media

Taya Govreen-Segal, Ehud Nakar, Kenta Hotokezaka +2

We present a quantitative model for the luminous fast blue optical transient AT2018cow in which a shock propagating through an aspherical circumstellar medium (CSM) produces the X-…