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Cited article:

The isolation of luminous blue variables resembles aging B-type supergiants, not the most massive unevolved stars

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Monthly Notices of the Royal Astronomical Society 489 (3) 4378 (2019)
https://doi.org/10.1093/mnras/stz2277

12CO and 13CO J = 3–2 observations toward N11 in the Large Magellanic Cloud

M. Celis Peña, S. Paron, M. Rubio, C. N. Herrera and M. E. Ortega
Astronomy & Astrophysics 628 A96 (2019)
https://doi.org/10.1051/0004-6361/201935446

LMC Blue Supergiant Stars and the Calibration of the Flux-weighted Gravity–Luminosity Relationship

M. A. Urbaneja, R.-P. Kudritzki, W. Gieren, G. Pietrzyński, F. Bresolin and N. Przybilla
The Astronomical Journal 154 (3) 102 (2017)
https://doi.org/10.3847/1538-3881/aa79a8

Swift J045106.8−694803: a highly magnetized neutron star in the Large Magellanic Cloud

H. Klus, E. S. Bartlett, A. J. Bird, et al.
Monthly Notices of the Royal Astronomical Society 428 (4) 3607 (2013)
https://doi.org/10.1093/mnras/sts304

New Massive Binaries in the Cygnus OB2 Association

Daniel C. Kiminki, M. Virginia McSwain and Henry A. Kobulnicky
The Astrophysical Journal 679 (2) 1478 (2008)
https://doi.org/10.1086/587777