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researcher

M. Ugalino

3 papers hereh-index 12 citations5 works total

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

author position
  • middle author2

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.GA1

identity via Semantic Scholar / OpenAlex

most citedUsing 44Ti Emission to Differentiate Between Thermonuclear Supernova Progenitors

6 citations · 6 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2026

Towards robust simulations of the galactic dynamo: a cross-code comparison between Eulerian and Lagrangian schemes

Mark Ivan Ugalino, Benedikt Diemer, Vadim A. Semenov +8

Galactic magnetic fields are thought to be seeded by microscopic processes such as the Biermann battery and are primarily amplified to observed microgauss strengths by dynamo proce…

astro-ph.HE2026

First-Principles Turbulence-Driven Deflagration-to-Detonation Transition Mechanism for Near-Chandrasekhar Mass White Dwarf Progenitors

Krut Patel, Akshay Dongre, Robert Fisher +4

Type Ia supernovae (SNe Ia) play an important role throughout astrophysics, most notably as standardizable cosmological candles. Yet, their stellar progenitors and explosion mechan…

astro-ph.HE2022★ 6 cited

Using 44Ti Emission to Differentiate Between Thermonuclear Supernova Progenitors

Daniel Kosakowski, Mark Ivan Ugalino, Robert Fisher +3

The radiosotope 44Ti is produced through α-rich freezeout and explosive helium burning in type Ia supernovae (SNe Ia). In this paper, we discuss how the detection of 44…

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