activity
20212026
most citedExplosion mechanism of core-collapse supernovae: role of the Si/O interface

53 citations · 318 across the 25 of their papers we have counts for

collaborators
Showing 2023Show all

4 papers · 1 filter

astro-ph.SR2023★ 40 cited

Zero and extremely low metallicity rotating massive stars: evolution, explosion, and nucleosynthesis up to the heaviest nuclei

Lorenzo Roberti, Marco Limongi, Alessandro Chieffi

We present the evolution and the explosion of two massive stars, 15 and 25 M, spanning a wide range of initial rotation velocities (from 0 to 800 km/s) and three initial…

astro-ph.SR2023★ 1 cited

Evolution and final fate of solar metallicity stars in the mass range 7-15 Msun. I. The transition from AGB to SAGB stars, Electron Capture and Core Collapse Supernovae progenitors

Marco Limongi, Lorenzo Roberti, Alessandro Chieffi +1

According to a standard initial mass function, stars in the range 7-12 Msun constitute ~50% (by number) of the stars more massive than ~7 Msun, but, in spite of this, their evoluti…

astro-ph.SR2023★ 32 cited

The -process nucleosynthesis in core-collapse supernovae. I. A novel analysis of -process yields in massive stars

L. Roberti, M. Pignatari, A. Psaltis +4

The -process nucleosynthesis in core-collapse supernovae is generally accepted as a feasible process for the synthesis of neutron-deficient isotopes beyond iron. However, crucia…

astro-ph.GA2023★ 51 cited

On the origin of the Galactic thin and thick discs, their abundance gradients and the diagnostic potential of their abundance ratios

Nikos Prantzos, Carlos Abia, Tianxiang Chen +8

Using a semi-analytical model of the evolution of the Milky Way, we show how secular evolution can create distinct overdensities in the phase space of various properties (e.g. age…