Neglecting the porosity of hot-star winds can lead to underestimating mass-loss rates
A&A, 476 3 (2007) 1331-1340
Published online: 2007-10-26
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Simultaneous X-ray and optical spectroscopy of the Oef supergiantλCephei
G. Rauw, A. Hervé, Y. Nazé, et al.Astronomy & Astrophysics 580 A59 (2015)
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2dF-AAOmega spectroscopy of massive stars in the Magellanic Clouds
C. J. Evans, J. Th. van Loon, R. Hainich and M. BaileyAstronomy & Astrophysics 584 A5 (2015)
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Mass loss from inhomogeneous hot star winds
J. O. Sundqvist, J. Puls and S. P. OwockiAstronomy & Astrophysics 568 A59 (2014)
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The evolution of massive stars and their spectra
Jose H. Groh, Georges Meynet, Sylvia Ekström and Cyril GeorgyAstronomy & Astrophysics 564 A30 (2014)
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The 100-monthSwiftcatalogue of supergiant fast X-ray transients
P. Romano, H. A. Krimm, D. M. Palmer, et al.Astronomy & Astrophysics 562 A2 (2014)
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