collaborators

5 papers

astro-ph.HE2025

Extreme anisotropies in deep layers of an exploding star: overabundance of Cr in the northeastern jet of Cassiopeia A

Vincenzo Sapienza, Marco Miceli, Masaomi Ono +5

Core-collapse supernovae drive nucleosynthesis under extreme thermodynamic conditions, and complex mechanisms are at work prompting the transport of heavy elements from deep stella…

astro-ph.HE2025

Measuring the initial mass of 44Ti in SN 1987A through the 44Sc emission line

Roberta Giuffrida, Marco Miceli, Emanuele Greco +7

Context. Deriving the mass and large-scale asymmetries of radioactive isotopes offers valuable insights into the complex phases of a supernova explosion. Important examples are $^{…

astro-ph.HE2025

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.HE2025

Origin of holes and rings in the Green Monster of Cassiopeia A: Insights from 3D magnetohydrodynamic simulations

S. Orlando, H. -T. Janka, A. Wongwathanarat +10

[Abridged] Cassiopeia A (Cas A) provides a unique opportunity to study supernova (SN) dynamics and interactions with the circumstellar medium (CSM). Recent JWST observations reveal…

astro-ph.HE2024

Constraining the CSM structure and progenitor mass-loss history of interacting supernovae through 3D hydrodynamic modeling: The case of SN 2014C

S. Orlando, E. Greco, R. Hirai +9

We investigate SN 2014C using three-dimensional hydrodynamic modeling, focusing on its early interaction with dense circumstellar medium (CSM). Our objective is to uncover the pre-…