activity
20152026
most citedNegative and Positive Feedback from a Supernova Remnant with SHREC: A detailed Study of the Shocked Gas in IC443

27 citations · 133 across the 14 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

5 papers · 1 filter

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.HE2025★ 8 cited

Tracing the ejecta structure of SN 1987A: Insights and diagnostics from 3D MHD simulations

S. Orlando, M. Miceli, M. Ono +14

Supernova (SN) 1987A provides a unique window into the aftermath of a massive stellar explosion, offering key insights into the ejecta's morphology, composition, explosion mechanis…

astro-ph.HE2020★ 4 cited

Modeling particle acceleration and non-thermal emission in supernova remnants

S. Orlando, M. Miceli, S. Ustamujic +5

According to the most popular model for the origin of cosmic rays (CRs), supernova remnants (SNRs) are the site where CRs are accelerated. Observations across the electromagnetic s…

astro-ph.HE2020★ 24 cited

Modeling the mixed-morphology supernova remnant IC 443. Origin of its complex morphology and X-ray emission

S. Ustamujic, S. Orlando, E. Greco +4

The morphology and the distribution of material observed in SNRs reflect the interaction of the SN blast wave with the ambient environment, the physical processes associated with t…

astro-ph.HE2020★ 16 cited

3D modeling from the onset of the SN to the full-fledged SNR: Role of an initial ejecta anisotropy on matter mixing

Antonio Tutone, Salvatore Orlando, Marco Miceli +8

The aim of this work is to bridge the gap between CC SNe and their remnants by investigating how post-explosion anisotropies in the ejecta influence the structure and chemical prop…