The “hidden” companion in LB-1 unveiled by spectral disentangling
A&A, 639 (2020) L6
Published online: 2020-07-10
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Velocity monitoring of γ Cas stars reveals their binarity status
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Gravitational Wave Sources in Our Galactic Backyard: Predictions for BHBH, BHNS, and NSNS Binaries Detectable with LISA
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The VLT-FLAMES survey of massive 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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Interferometric Detections of sdO Companions Orbiting Three Classical Be Stars
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Observational Imprints of Binary Evolution on B- and Be-star Populations
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The spins of stripped B stars support magnetic internal angular momentum transport
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NGC 2004 #115: a black hole imposter containing three luminous stars
Kareem El-Badry, Kevin B Burdge and Przemek MrózMonthly Notices of the Royal Astronomical Society 511 (2) 3089 (2022)
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Parameters of the eclipsing binary α Draconis observed by TESS and SONG
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Discovery of post-mass-transfer helium-burning red giants using asteroseismology
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A Sun-like star orbiting a black hole
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To be or not to be a black hole: detailed binary population models as a sanity check
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The ‘Giraffe’: discovery of a stripped red giant in an interacting binary with an ∼2 M⊙ lower giant
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Binaries with Possible Compact Components Discovered from the LAMOST Time-domain Survey of Four K2 Plates
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Ups!... I did it again: unveiling the hidden companion in Upsilon Sagittarii, a unique binary system at a second mass transfer stage
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An X-ray-quiet black hole born with a negligible kick in a massive binary within the Large Magellanic Cloud
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Overview of the LAMOST survey in the first decade
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HR 6819 is a binary system with no black hole
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The Tarantula Massive Binary Monitoring
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Properties of the Be-type stars in 30 Doradus
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https://doi.org/10.1093/mnras/stac630
NGC 1850 BH1 is another stripped-star binary masquerading as a black hole
Kareem El-Badry and Kevin B BurdgeMonthly Notices of the Royal Astronomical Society: Letters 511 (1) 24 (2022)
https://doi.org/10.1093/mnrasl/slab135
Cygnus X-1 contains a 21–solar mass black hole—Implications for massive star winds
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