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20022009
most citedThe surprising magnetic topology of tauSco: fossil remnant or dynamo output?

496 citations · 1.1k across the 7 of their papers we have counts for

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astro-ph200840 cited

A Three-Decade Outburst of the LMC Luminous Blue Variable R127 Draws to a Close

Nolan R. Walborn, Otmar Stahl, Roberto C. Gamen +7

The paradigmatic Luminous Blue Variable R127 in the Large Magellanic Cloud has been found in the intermediate, peculiar early-B state, and substantially fainter in visual light, si…

astro-ph200871 cited

The weak magnetic field of the O9.7 supergiant zeta Orionis A

J. -C. Bouret, J. -F. Donati, F. Martins +4

We report here the detection of a weak magnetic field of 50 - 100 G on the O9.7 supergiant zeta Ori A, using spectropolarimetric observations obtained with NARVAL at the 2m Telesco…

astro-ph200630 cited

Towards an understanding of the Of?p star HD191612: Phase-resolved multiwavelength observations

Yael Naze, Gregor Rauw, A. M. T. Pollock +2

We present the analysis of phase-resolved X-ray and optical observations of the peculiar hot star HD191612 (Of?p). This star is known to display line-profile variations that are re…

astro-ph2006496 cited

The surprising magnetic topology of tauSco: fossil remnant or dynamo output?

JF Donati, ID Howarth, MM Jardine +9

We report the discovery of a medium-strength (~0.5kG) magnetic field on the young, massive star tauSco (B0.2V), which becomes the third-hottest magnetic star known. Circularly pola…

astro-ph2006263 cited

Bright OB stars in the Galaxy - III. Constraints on the radial stratification of the clumping factor in hot star winds from a combined Halpha, IR and radio analysis

J. Puls, N. Markova, S. Scuderi +4

Recent results strongly challenge the canonical picture of massive star winds: various evidence indicates that currently accepted mass-loss rates, Mdot, may need to be revised down…

astro-ph2004

FUSE Observations of Variability in Hot-Star Winds

A. W. Fullerton, D. L. Massa, R. K. Prinja +3

New constraints on the large-scale wind structures responsible for discrete absorption components are obtained from far-ultraviolet time-series observations of O supergiants in the…