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Home All issues A&A, 388 2 (2002) 587-608 Article references

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Cited article:

Wind-line Variability and Intrinsic Errors in Observational Mass-loss Rates

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The wind of rotating B supergiants – II. The δ-slow hydrodynamic regime

R O J Venero, M Curé, J Puls, L S Cidale, M Haucke, I Araya, A Gormaz-Matamala and C Arcos
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Optically thick structure in early B-type supergiant stellar winds at low metallicities

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Monthly Notices of the Royal Astronomical Society 527 (4) 11422 (2023)
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Coordinated UV and X-Ray Spectroscopic Observations of the O-type Giant ξ Per: The Connection between X-Rays and Large-scale Wind Structure* †

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METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble Program. I. Overview and Initial Results

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Demonstration of a Novel Method for Measuring Mass-loss Rates for Massive Stars

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Mass-loss rates from mid-infrared excesses in LMC and SMC O stars

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Probing the Outflowing Multiphase Gas ∼1 kpc below the Galactic Center

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Studying the photometric and spectroscopic variability of the magnetic hot supergiant ζ Orionis Aa

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Astronomy & Astrophysics 602 A91 (2017)
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X-ray, UV and optical analysis of supergiants: ϵ Ori

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Metallicity dependence of turbulent pressure and macroturbulence in stellar envelopes

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INVESTIGATING NEARBY STAR-FORMING GALAXIES IN THE ULTRAVIOLET WITHHST/COS SPECTROSCOPY. I. SPECTRAL ANALYSIS AND INTERSTELLAR ABUNDANCE DETERMINATIONS

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

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The Astronomical Journal 141 (4) 120 (2011)
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Structure and clumping in the fast wind of NGC 6543

R. K. Prinja, S. E. Hodges, D. L. Massa, A. W. Fullerton and A. W. Burnley
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Multi-periodic photospheric pulsations and connected wind structures in HD 64760

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The superimposed photospheric and stellar wind variability of the O-type supergiant $\mathsf{\alpha}$ Camelopardalis

R. K. Prinja, N. Markova, S. Scuderi and H. Markov
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Looking for Discrete UV Absorption Features in the Early‐Type Eclipsing Binariesμ1Scorpii and AO Cassiopeiae

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Kinematic model inversions of hot star recurrent DAC data – tests against dynamical CIR models

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Astronomy & Astrophysics 417 (3) 1039 (2004)
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Terminal Velocities of Luminous, Early‐Type Stars in the Small Magellanic Cloud

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Inference of hot star density stream properties from data on rotationally recurrent DACs

J. C. Brown, R. K. Barrett, L. M. Oskinova, et al.
Astronomy & Astrophysics 413 (3) 959 (2004)
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Quantitative Studies of the Far‐Ultraviolet, Ultraviolet, and Optical Spectra of Late O‐ and Early B‐Type Supergiants in the Magellanic Clouds

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Large-scale wind structures in OB supergiants: a search for rotationally modulated Hα variability

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Monthly Notices of the Royal Astronomical Society 351 (2) 552 (2004)
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