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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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Showing 2021Show all

7 papers · 1 filter

astro-ph.SR2021★ 5 cited

Binary-object spectral-synthesis in 3D (BOSS-3D) -- Modelling H-alpha emission in the enigmatic multiple system LB-1

L. Hennicker, N. D. Kee, T. Shenar +5

Context: To quantitatively decode the information stored within an observed spectrum, detailed modelling of the physical state and accurate radiative transfer solution schemes are…

astro-ph.SR2021★ 9 cited

The Carina High-contrast Imaging Project for massive Stars (CHIPS): II. O stars in Trumpler~14

Alan Rainot, Maddalena Reggiani, Hugues Sana +2

Most massive stars belong to multiple systems, yet the formation process leading to such high multiplicity remains insufficiently understood. To help constrain the different format…

astro-ph.SR2021★ 11 cited

Dynamical parallax, physical parameters and evolutionary status of the components of the bright eclipsing binary α Draconis

K. Pavlovski, C. A. Hummel, A. Tkachenko +13

Altough both components of the bright eclipsing binary Dra having been resolved using long baseline interferometry and the secondary component shown to contribute some 15\% of…

astro-ph.SR2021★ 4 cited

LBV phenomenon and binarity: The environment of HR Car

A. Mehner, S. Janssens, C. Agliozzo +7

Luminous blue variable stars (LBVs) are of great interest in massive-star evolution as they experience very high mass-loss episodes within short periods of time. HR Car is a famous…

astro-ph.SR2021★ 2 cited

The observed multiplicity properties of B-type stars in the Galactic young open cluster NGC 6231

G. Banyard, H. Sana, L. Mahy +3

It is well known that massive O-stars are frequently (if not always) found in binary or higher-order multiple systems, but this fact has been less robustly investigated for the low…

astro-ph.SR2021★ 55 cited

The young massive SMC cluster NGC 330 seen by MUSE II. Multiplicity properties of the massive-star population

J. Bodensteiner, H. Sana, C. Wang +10

Observations of massive stars in young open clusters (< ~8 Myr) have shown that a majority of them are in binary systems, most of which will interact during their life. Populations…