collaborators

12 papers

physics.plasm-ph2026

Efficient ion re-acceleration in laboratory-produced interpenetrating collisionless shocks

W. Yao, I. Cohen, P. Suarez Gerona +20

Although the origin of cosmic rays (CRs) remains an open question, collisionless magnetized shock waves are widely regarded as key sites for particle acceleration. Recent theories…

astro-ph.HE2026

Supernova remnants in the new radio astronomy era

A. Ingallinera, M. Arias, G. Castelletti +25

Supernova remnants (SNRs) are what is left after stellar explosions, when the stellar ejecta, the explosion shock and the circumstellar medium interact. Despite being among the fir…

astro-ph.SR2026

Evolved massive stars and their impact on their environment

C. S. Buemi, G. Umana, C. Trigilio +15

The comprehension of the final stages of massive star evolution and their path toward the eventual supernova explosion necessarily involves the study of stellar winds and the circu…

astro-ph.HE2026

Probing the potential high-energy messengers of the anticipated T Coronae Borealis outburst

O. Petruk, T. Kuzyo, S. Orlando +4

T Coronae Borealis (T CrB) is a nearby recurrent nova expected to erupt in the near future, offering a unique opportunity to study particle acceleration and high-energy emission fr…

astro-ph.SR2026

A New Catalogue of Galactic Red Supergiants for direct detection of episodic mass-loss events

M. Lauriano, F. Bocchino, M. Miceli +5

We present GalRSG, a new catalogue of 227 Galactic Red Supergiants in the Scutum-Crux region, which provides a nearly coeval and co-distant sample, target of a long-term, panchroma…

astro-ph.HE2026

Deciphering the Remnants of Core-Collapse Supernovae: Reconstructing Progenitor Star Properties and Explosion Mechanisms

Salvatore Orlando

(Abridged) Recent JWST observations of Cassiopeia A (Cas A) reveal unprecedented ejecta substructure, including a web of filaments and the enigmatic "Green Monster" (GM), character…