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researcher

Michael Bertolli

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author1
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3

identity via Semantic Scholar / OpenAlex

most citedAdvanced burning stages and fate of 8-10 Mo stars

202 citations · 323 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2015★ 104 cited

H ingestion into He-burning convection zones in super-AGB stellar models as a potential site for intermediate neutron-density nucleosynthesis

S. Jones, C. Ritter, F. Herwig +4

We investigate the evolution of super-AGB thermal pulse (TP) stars for a range of metallicities (Z) and explore the effect of convective boundary mixing (CBM). With decreasing meta…

astro-ph.SR2013★ 17 cited

Systematic and correlated nuclear uncertainties in the i-process at the neutron shell closure N = 82

M. G. Bertolli, F. Herwig, M. Pignatari +1

Nuclear astrophysics simulations aiming to study the origin of the elements in stars require a multitude of nuclear physics input. Both systematic model dependent and statistically…

astro-ph.SR2013★ 202 cited

Advanced burning stages and fate of 8-10 Mo stars

Samuel Jones, Raphael Hirschi, Ken'ichi Nomoto +9

The stellar mass range 8<M/Mo<12 corresponds to the most massive AGB stars and the most numerous massive stars. It is host to a variety of supernova progenitors and is therefore ve…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.