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20152026
most citedThe 'hidden' companion in LB-1 unveiled by spectral disentangling

132 citations · 1.5k across the 59 of their papers we have counts for

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16 papers · 1 filter

astro-ph.SR2025

The Triple System V1371 Tau: An Eclipsing Binary with an Outer Be Star

Danilo F. Rocha, Marcelo Emilio, Jonathan Labadie-Bartz +10

Although triple systems are common, their orbital dynamics and stellar evolution remain poorly understood. We investigated the V1371 Tau system using TESS photometry, multi-epoch s…

astro-ph.SR2025

HR6819: a puffed-up stripped star system challenging stable mass transfer theory

A. Picco, P. Marchant, H. Sana +8

HR6819 is the first system with a puffed-up low mass stripped star and a classical Be star whose nature has been confirmed by optical interferometry. It shows the most extreme mass…

astro-ph.SR2025★ 22 cited

A high fraction of close massive binary stars at low metallicity

H. Sana, T. Shenar, J. Bodensteiner +74

At high metallicity, a majority of massive stars have at least one close stellar companion. The evolution of such binaries is subject to strong interaction processes, heavily impac…

astro-ph.SR2025

Astrophotometric search for massive stars in the Milky way. Confronting Random Forest predictions with available spectroscopy

N. Monsalves, A. Bayo, M. Jaque Arancibia +4

Massive stars play a significant role in different branches of astronomy, from shaping the processes of star and planet formation to influencing the evolution and chemical enrichme…

astro-ph.SR2025

Binarity at LOw Metallicity (BLOeM): Pipeline-Determined Physical Properties of OB Stars

J. M. Bestenlehner, Paul A. Crowther, V. A. Bronner +8

We aim to determine the physical properties of OB stars from the multi-epoch VLT/FLAMES BLOeM spectroscopic survey of the Small Magellanic Cloud. We apply a pipeline designed to an…

astro-ph.SR2025

Characterisation of B-type stars in four young Galactic open clusters. I. Stellar content and binary properties

Federica Nardini, Julia Bodensteiner, Hugues Sana +3

Multiplicity among massive stars represents a major uncertainty in stellar evolution theory, because the extra physical processes that it introduces significantly impacts each star…