collaborators

8 papers

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.IM2025

ESO Expanding Horizons: Underluminous Thermonuclear Supernovae

Paul J. Groot, Simone Scaringi, Nancy Elias-Rosa

Underluminous Thermonuclear Supernovae (uTSNe) are an emerging class of transient events that resemble classic Supernovae Type Ia, but peak at much lower luminosities. Suspected to…

astro-ph.IM2025

The final stages of binary evolution using multi-messenger studies

Thomas Kupfer, Simone Scaringi, Paul Groot +11

Ultracompact Galactic binaries with orbital periods below an hour are among the strongest persistent gravitational-wave (GW) sources in the mHz band and will constitute the dominan…

astro-ph.IM2025

Nova Explosions in 2040

Alessandro Ederoclite, Domitilla De Martino, Paul Groot +7

Novae are thermonuclear explosions on the surface of accreting white dwarfs and are key laboratories for studying explosive nucleosynthesis, particle acceleration, shock physics, a…

astro-ph.HE2025

GRBs and Relativistic Transients in the 2040s

Nikhil Sarin, Andrew Levan, Nial Tanvir +9

Relativistic transients such as gamma-ray bursts (GRBs), jetted tidal disruption events, luminous fast blue optical transients, and fast X-ray transients, represent the brightest e…

astro-ph.IM2025

Luminous Fast Blue Optical Transients in the 2040s

A. A. Chrimes, N. Sarin, D. Coppejans +6

Luminous Fast Blue Optical Transients (LFBOTs) are a class of extragalactic transient of uncertain origin. Several hypotheses have been put forward which could feasibly be consiste…