collaborators

15 papers

astro-ph.SR2026

The Long-Period Radio Transient and Cataclysmic Variable ASKAP J1745-5051: Evidence for a 15,000 K White Dwarf and a Sub-Stellar Donor

Christian Knigge, Simone Scaringi, Noel Castro Segura +2

Long-period transients (LPTs) are radio sources that exhibit polarized periodic radio bursts on time-scales of minutes to hours. At least some LPTs are associated with white dwarfs…

astro-ph.HE2026

Radiation-ionization hydrodynamic simulations of AGN line-driven winds lead to transient shielding and BAL/UFO signatures

Nicolas Scepi, Christian Knigge, Amin Mosallanezhad +4

Disc winds from active galactic nuclei (AGN) can be launched by radiation pressure acting on spectral lines. However, launching a line-driven wind in the X-ray rich environment of…

astro-ph.SR2026

The Inner and Outer Shock Layers of Bow Shocks in Cataclysmic Variables

Krystian Ilkiewicz, Christian Knigge, Simone Scaringi +3

Bow shocks around cataclysmic variables (CVs) have traditionally been identified with a single bright optical arc. This feature has been interpreted as the bow shock formed by the…

astro-ph.HE2026

Accreting White Dwarfs: An Unreview

Simone Scaringi, Christian Knigge, Domitilla de Martino

Accreting white dwarfs (AWDs) are among the best natural laboratories for understanding disk accretion. Their proximity, brightness, and purely classical nature make them ideal sys…

astro-ph.SR2026

A persistent bow shock in a diskless magnetised accreting white dwarf

Krystian Ilkiewicz, Simone Scaringi, Domitilla de Martino +9

Stellar bow shocks are formed when an outflow interacts with the interstellar medium. In white dwarfs accreting from a binary companion, outflows are associated with either strong…

astro-ph.HE2026

A comprehensive search for high-velocity X-ray sources: New compact object binary candidates in the Gaia era

Yue Zhao, Poshak Gandhi, Christian Knigge +6

We perform a comprehensive search for high-velocity X-ray sources with large X-ray/optical flux ratios (), identifying candidates for interacting black h…