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Cited article:

Combined spectroscopy and intensity interferometry to determine the distances of the blue supergiants P Cygni and Rigel

E S G de Almeida, M Hugbart, A Domiciano de Souza, et al.
Monthly Notices of the Royal Astronomical Society 515 (1) 1 (2022)
https://doi.org/10.1093/mnras/stac1617

5 yr of BRITE-Constellation photometry of the luminous blue variable P Cygni: properties of the stochastic low-frequency variability

Ashley Elliott, Noel D Richardson, Herbert Pablo, et al.
Monthly Notices of the Royal Astronomical Society 509 (3) 4246 (2021)
https://doi.org/10.1093/mnras/stab3112

Intensity interferometry of P Cygni in the H α emission line: towards distance calibration of LBV supergiant stars

W Guerin, R Kaiser, D Vernet, et al.
Monthly Notices of the Royal Astronomical Society 494 (1) 218 (2020)
https://doi.org/10.1093/mnras/staa588

THEH-BAND EMITTING REGION OF THE LUMINOUS BLUE VARIABLE P CYGNI: SPECTROPHOTOMETRY AND INTERFEROMETRY OF THE WIND

N. D. Richardson, G. H. Schaefer, D. R. Gies, et al.
The Astrophysical Journal 769 (2) 118 (2013)
https://doi.org/10.1088/0004-637X/769/2/118

THE Hα VARIATIONS OF THE LUMINOUS BLUE VARIABLE P CYGNI: DISCRETE ABSORPTION COMPONENTS AND THE SHORT S DORADUS-PHASE

N. D. Richardson, N. D. Morrison, D. R. Gies, et al.
The Astronomical Journal 141 (4) 120 (2011)
https://doi.org/10.1088/0004-6256/141/4/120

Properties of the P Cygni wind found using the Self Absorption Curve method

G. Muratorio, N. Markova, M. Friedjung and G. Israelian
Astronomy & Astrophysics 390 (1) 213 (2002)
https://doi.org/10.1051/0004-6361:20020708