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Cited article:

Estimating the Structure and Geometry of Winds from Luminous Blue Variables via Fitting the Continuum Energy Distributions

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The Astrophysical Journal 659 (2) 1563 (2007)
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Neglecting the porosity of hot-star winds can lead to underestimating mass-loss rates

L. M. Oskinova, W.-R. Hamann and A. Feldmeier
Astronomy & Astrophysics 476 (3) 1331 (2007)
https://doi.org/10.1051/0004-6361:20066377

A Clumping-independent Diagnostic of Stellar Mass-Loss Rates: Rapid Clump Destruction in Adiabatic Colliding Winds

J. M. Pittard
The Astrophysical Journal 660 (2) L141 (2007)
https://doi.org/10.1086/518365

The Local Environments of Long‐Duration Gamma‐Ray Bursts

Patrick A. Young and Chris L. Fryer
The Astrophysical Journal 670 (1) 584 (2007)
https://doi.org/10.1086/521695

The VLT-FLAMES survey of massive stars: wind properties and evolution of hot massive stars in the Large Magellanic Cloud

M. R. Mokiem, A. de Koter, C. J. Evans, et al.
Astronomy & Astrophysics 465 (3) 1003 (2007)
https://doi.org/10.1051/0004-6361:20066489

Neon Abundances from aSpitzer/IRS Survey of Wolf‐Rayet Stars

R. Ignace, J. P. Cassinelli, G. Tracy, E. Churchwell and H. J. G. L. M. Lamers
The Astrophysical Journal 669 (1) 600 (2007)
https://doi.org/10.1086/521718

Spectroscopy of SMC Wolf-Rayet Stars Suggests that Wind Clumping Does Not Depend on Ambient Metallicity

S. V. Marchenko, C. Foellmi, A. F. J. Moffat, et al.
The Astrophysical Journal 656 (2) L77 (2007)
https://doi.org/10.1086/512725

The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars

M. R. Mokiem, A. de Koter, J. S. Vink, et al.
Astronomy & Astrophysics 473 (2) 603 (2007)
https://doi.org/10.1051/0004-6361:20077545

The Effect of Porosity on X‐Ray Emission‐Line Profiles from Hot‐Star Winds

Stanley P. Owocki and David H. Cohen
The Astrophysical Journal 648 (1) 565 (2006)
https://doi.org/10.1086/505698

Measurements and Analysis of Helium‐like Triplet Ratios in the X‐Ray Spectra of O‐Type Stars

Maurice A. Leutenegger, Frits B. S. Paerels, Steven M. Kahn and David H. Cohen
The Astrophysical Journal 650 (2) 1096 (2006)
https://doi.org/10.1086/507147