collaborators

8 papers

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.HE2026

On the acceleration of cosmic rays at the post-adiabatic shocks of supernova remnants

O. Petruk, R. Bandiera, T. Kuzyo +2

When a supernova remnant (SNR) interacts with the dense material of an interstellar cloud, its shock wave decelerates rapidly, and the post-shock temperature drops to levels that p…

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.HE2025

Predicting the X-ray signatures of the imminent T Coronae Borealis outburst through 3D hydrodynamic modeling

S. Orlando, L. Chomiuk, J. Drake +3

T Coronae Borealis (T CrB) is a symbiotic recurrent nova with eruptions in 1866 and 1946. Mounting evidence suggests an imminent outburst, offering a rare opportunity to observe a…

astro-ph.HE2025

On the properties of turbulence in the remnant of Tycho supernova

Oleh Petruk, Taras Kuzyo

We investigate the turbulent structures in the Tycho supernova remnant (SNR) by applying two-point autocorrelation and power spectral analyses to high-resolution X-ray and radio im…