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19982025
most citedThe Type IIb Supernova 2011dh from a Supergiant Progenitor

245 citations · 2.3k across the 49 of their papers we have counts for

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6 papers · 1 filter

astro-ph.HE2024

The impact of different magnetic braking prescriptions on the evolution of LMXBs

M. Echeveste, M. L. Novarino, O. G. Benvenuto +1

We revisit the evolution of low-mass close binary systems under different magnetic braking (MB) prescriptions. We study binaries with a neutron star accretor. During mass transfer…

astro-ph.HE2018★ 1 cited

Does PSR J1417-4402 system behave as a "Redback"?

M. A. De Vito, J. E. Horvath, O. G. Benvenuto

We study the present evolutionary status of the binary system containing the 2.66 ms pulsar PSR J1417-4402 in a 5.4 day orbit. This is the pulsar in the original source 3FGL J1417.…

astro-ph.HE2016★ 66 cited

The Unusual Super-Luminous Supernovae SN 2011kl and ASASSN-15lh

Melina C. Bersten, Omar G. Benvenuto, Mariana Orellana +1

Two recently discovered very luminous supernovae (SNe) present stimulating cases to explore the extents of the available theoretical models. SN 2011kl represents the first detectio…

astro-ph.HE2015★ 30 cited

Final Evolution and Delayed Explosions of Spinning White Dwarfs in Single Degenerate Models for Type Ia Supernovae

Omar G. Benvenuto, Jorge A. Panei, Ken'ichi Nomoto +2

We study the occurrence of delayed SNe~Ia in the single degenerate (SD) scenario. We assume that a massive carbon-oxygen (CO) white dwarf (WD) accretes matter coming from a compani…

astro-ph.HE2013

The Evolution of Proto-Strange Stars

Omar G. Benvenuto, J. E. Horvath

We perform 1D calculations of neutrino opacities inside a young "strange star" assumed to be the result of the conversion process of a normal neutron object. We evaluate the delept…

astro-ph.HE2012★ 245 cited

The Type IIb Supernova 2011dh from a Supergiant Progenitor

Melina C. Bersten, Omar G. Benvenuto, Ken'ichi Nomoto +10

A set of hydrodynamical models based on stellar evolutionary progenitors is used to study the nature of SN 2011dh. Our modeling suggests that a large progenitor star ---with R ~200…