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Cited article:

The structure of blue supergiant winds and the accretion in supergiant high-mass X-ray binaries

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Monthly Notices of the Royal Astronomical Society 398 (4) 2152 (2009)
https://doi.org/10.1111/j.1365-2966.2009.15265.x

Sub-surface convection zones in hot massive stars and their observable consequences

M. Cantiello, N. Langer, I. Brott, et al.
Astronomy & Astrophysics 499 (1) 279 (2009)
https://doi.org/10.1051/0004-6361/200911643

Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars

C. Aerts, J. Puls, M. Godart and M.-A. Dupret
Astronomy & Astrophysics 508 (1) 409 (2009)
https://doi.org/10.1051/0004-6361/200810471

Modeling Ultraviolet Wind Line Variability in Massive Hot Stars

A. Lobel and R. Blomme
The Astrophysical Journal 678 (1) 408 (2008)
https://doi.org/10.1086/529129

ChandraObservation of Cir X‐1 near the Periastron Passage: Evidence for an X‐Ray Jet?

R. Iaria, A. D’Ai, G. Lavagetto, et al.
The Astrophysical Journal 673 (2) 1033 (2008)
https://doi.org/10.1086/524311

Photometric Variability of the B8Iae Supergiant Variable HD 199478 (HR 8020)

John R. Percy, Rohan Palaniappan, Rajiv Seneviratne, Saul J. Adelman and Nevena Markova
Publications of the Astronomical Society of the Pacific 120 (865) 311 (2008)
https://doi.org/10.1086/529410

An alternative hypothesis for the outburst mechanism in supergiant fast X-ray transients: the case of IGR J11215–5952

L. Sidoli, P. Romano, S. Mereghetti, et al.
Astronomy & Astrophysics 476 (3) 1307 (2007)
https://doi.org/10.1051/0004-6361:20078137