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20002026
most citedSimultaneous formation of Solar System giant planets

48 citations · 200 across the 12 of their papers we have counts for

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Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR2026

On the origin of the short-period Blue Straggler Stars in Collinder 261: a binary evolution approach

M. Echeveste, M. J. Rain, G. Carraro +3

Building on the recent publication of a fresh catalog of blue straggler stars in Galactic open clusters using Gaia DR3, we conduct a study focusing on the blue straggler stars with…

astro-ph.SR2026

The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars

C. Martínez-Sebastián, R. Gamen, O. G. Benvenuto +6

For decades, the origin of helium enrichment in O-type stars has remained an open question. In this study, we investigate the correlation between surface helium abundance and orbit…

astro-ph.SR2026

Impact of stellar rotation on type II supernova progenitor masses from pre-explosion imaging

L. Martinez, O. G. Benvenuto, M. A. De Vito

The initial masses of red supergiant (RSG) type II supernova (SN II) progenitors are commonly inferred from pre-explosion imaging by converting the progenitor luminosity into an in…

astro-ph.SR2024

Binary origin of blue straggler stars in Galactic star clusters

M. J. Rain, M. S. Pera, G. Perren +5

Building on the recent release of a new \emph{Gaia}-based blue straggler star catalog in Galactic open star clusters (OCs), we explored the properties of these stars in a cluster s…

astro-ph.SR2013★ 19 cited

Apsidal motion in massive close binary systems. I. HD 165052 an extreme case?

G. Ferrero, R. Gamen, O. G. Benvenuto +1

We present a new set of radial-velocity measurements of the spectroscopic binary HD 165052 obtained by disentangling of high-resolution optical spectra. The longitude of the perias…

astro-ph.SR2012★ 14 cited

The evolution of low mass, close binary systems with a neutron star component: a detailed grid

M. A. De Vito, O. G. Benvenuto

In close binary systems composed of a normal, donor star and an accreting neutron star, the amount of material received by the accreting component is, so far, a real intrigue. In t…

astro-ph.SR2012

Evolution of low mass close binary systems with a neutron star: its dependence with the initial neutron star mass

M. A. De Vito, O. G. Benvenuto

We construct a set of binary evolutionary sequences for systems composed by a normal, solar composition, donor star together with a neutron star. We consider a variety of masses fo…