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20012023
most citedThe MiMeS Survey of Magnetism in Massive Stars: Introduction and overview

232 citations · 984 across the 19 of their papers we have counts for

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13 papers · 1 filter

astro-ph.SR2023

Modeling Variable Linear Polarization Produced by Co-Rotating Interaction Regions (CIRs) Across Optical Recombination Lines of Wolf-Rayet Stars

R Ignace, J E Bjorkman, A-N Chene +5

Massive star winds are structured both stochastically ("clumps") and often coherently (Co-rotation Interaction Regions, or CIRs). Evidence for CIRs threading the winds of Wolf-Raye…

astro-ph.SR2023★ 41 cited

X-Shooting ULLYSES: Massive stars at low metallicity. III. Terminal wind speeds of ULLYSES massive stars

C. Hawcroft, H. Sana, L. Mahy +26

The winds of massive stars have an impact on stellar evolution and on the surrounding medium. The maximum speed reached by these outflows, the terminal wind speed, is a global wind…

astro-ph.SR2023★ 7 cited

Spectrum of the secondary component and new orbital elements of the massive triple star Delta Ori A

A. Oplištilová, P. Mayer, P. Harmanec +13

Orionis is the closest massive multiple stellar system and one of the brightest members of the Orion OB association. The primary (Aa1) is a unique evolved O star. In this work,…

astro-ph.SR2020★ 7 cited

An extensive spectroscopic time series of three Wolf-Rayet stars -- II. A search for wind asymmetries in the dust-forming WC7 binary WR137

N. St-Louis, C. Piaulet, N. D. Richardson +39

We present the results of a four-month, spectroscopic campaign of the Wolf-Rayet dust-making binary, WR137. We detect only small-amplitude, random variability in the CIII5696 emiss…

astro-ph.SR2019★ 67 cited

The Tarantula Massive Binary Monitoring: III. Atmosphere analysis of double-lined spectroscopic systems

L. Mahy, H. Sana, M. Abdul-Masih +17

Accurate stellar parameters of individual objects in binary systems are essential to constrain the effects of binarity on stellar evolution. These parameters serve as a prerequisit…

astro-ph.SR2016★ 19 cited

VLTI-AMBER velocity-resolved aperture-synthesis imaging of Eta Carinae with a spectral resolution of 12000. Studies of the primary star wind and innermost wind-wind collision

G. Weigelt, K. -H. Hofmann, D. Schertl +26

Context. The mass loss from massive stars is not understood well. Eta Car is a unique object for studying the massive stellar wind during the LBV phase. It is also an eccentric bin…