2 papers
astro-ph.HE2025
Modeling the circumstellar interaction around SN 2004gq
A. P. Nagy, B. H. Pál, T. Szalai
The relationship between the mass-loss history and final evolutionary stage of massive stars and the properties of the observable supernova (SN) is still under debate. This is espe…
astro-ph.HE2025
Can circumstellar interaction explain the strange light curve features of Type Ib/c supernovae?
Andrea P. Nagy, Zsofia R. Bodola
Context. The evolution and the surrounding of stripped-envelope supernova progenitors are still under debate: some studies suggest single-star, while others prefer massive binary p…