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Cited article:

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Boron Abundances in Early B Dwarfs of the Galactic Open Cluster NGC 3293*

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The Progenitors of Be-stars Paired with O-subdwarfs: The Spin-up of a Be Star at the Stage of Conservative Mass Exchange

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Binarity at LOw Metallicity (BLOeM)

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MWC 656 is unlikely to contain a black hole

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Gaia uncovers difference in B and Be star binarity at small scales: evidence for mass transfer causing the Be phenomenon

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Nitrogen abundances of the Be-type stars in 30 Doradus

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Population synthesis of Be X-ray binaries: metallicity dependence of total X-ray outputs

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Monthly Notices of the Royal Astronomical Society 527 (3) 5023 (2023)
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The young massive SMC cluster NGC 330 seen by MUSE

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Hubble Space Telescope survey of Magellanic Cloud star clusters: UV-dim stars in young clusters

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The initial spin distribution of B-type stars revealed by the split main sequences of young star clusters

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The B-type Binaries Characterisation Programme – II. VFTS 291: a stripped star from a recent mass transfer phase

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Gamma Cas Stars as Be+White Dwarf Binary Systems

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Formation and Destiny of White Dwarf and Be Star Binaries

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Classical OBe Stars as Post-supernova Runaways: Confirming Binary Origins

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Ultraviolet Spectropolarimetry: on the origin of rapidly rotating B stars

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Interferometric Detections of sdO Companions Orbiting Three Classical Be Stars

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Birth of a Be star: an APOGEE search for Be stars forming through binary mass transfer

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The effects of stellar rotation along the main sequence of the 100-Myr-old massive cluster NGC 1850

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The Spin-up of a Star Gaining Mass in a Close Binary System on the Thermal Time Scale

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Properties of the Be-type stars in 30 Doradus

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V1294 Aql = HD 184279: A bad boy among Be stars or an important clue to the Be phenomenon?

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A census of OBe stars in nearby metal-poor dwarf galaxies reveals a high fraction of extreme rotators

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Observational Imprints of Binary Evolution on B- and Be-star Populations

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Partial-envelope stripping and nuclear-timescale mass transfer from evolved supergiants at low metallicity

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Velocity monitoring of γ Cas stars reveals their binarity status

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Evolution of Accretor Stars in Massive Binaries: Broader Implications from Modeling ζ Ophiuchi

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Growth and dissipation of Be star discs in misaligned binary systems

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