Ejecta clumps revealed by study of reverse-shocked ejecta through MUSE integral field spectroscopy of SNR 0509-67.5

arXiv:2608.17465 · astro-ph.SR, astro-ph.GA, astro-ph.HE · Submitted 2026-08-18 · Read on arXiv

astro-ph.SR, astro-ph.GA, astro-ph.HE

Submitted: 2026-08-18

Updated: 2026-08-18

Terminology

• Core — 4× in this paper · explained in 2 episodes
• Trace — 3× in this paper · explained in 2 episodes
• Ablation — 1× in this paper · explained in 1 episode
• Aperture — 1× in this paper · explained in 1 episode

Related papers

• HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager
• Effect of Neutron Star Jets on Common Envelope Evolution
• Constraining the origin of magnetic white dwarfs
• JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting
• Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics
• Can MHD Oscillations Modulate Quasi-Periodic Plasma Release from Coronal Streamers?