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20032022
most citedThe surprising magnetic topology of tauSco: fossil remnant or dynamo output?

496 citations · 2.1k across the 45 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.SR20195 cited

No evidence of a sudden change of spectral appearance or magnetic field strength of the O9.7V star HD 54879

G. A. Wade, S. Bagnulo, Z. Keszthelyi +8

It was recently claimed that the magnetic O-type star HD 54879 exhibits important radial velocity variability indicative of its presence in a spectroscopic binary. More remarkably,…

astro-ph.SR2019

The Magnetic Early B-type Stars III: A main sequence magnetic, rotational, and magnetospheric biography

M. E. Shultz, G. A. Wade, Th. Rivinius +10

Magnetic confinement of stellar winds leads to the formation of magnetospheres, which can be sculpted into Centrifugal Magnetospheres (CMs) by rotational support of the corotating…

astro-ph.SR2019

The MiMeS survey of Magnetism in Massive Stars: Magnetic properties of the O-type star population

V. Petit, G. A. Wade, F. R. N. Schneider +5

In this paper, we describe an analysis of the MiMeS Survey of O-type stars to explore the range of dipolar field strengths permitted by the polarisation spectra that do not yield a…

astro-ph.SR201922 cited

Lupi: measuring the heartbeat of a doubly-magnetic massive binary with BRITE-Constellation

H. Pablo, M. Shultz, J. Fuller +15

Lupi A is a binary system consisting of two main sequence early B-type stars Aa and Ab in a short period, moderately eccentric orbit. The close binary pair is the onl…

astro-ph.SR201914 cited

Investigating the origin of the spectral line profiles of the Hot Wolf-Rayet Star WR2

A. -N. Chené, N. St-Louis, A. F. J. Moffat +12

The hot WN star WR2 (HD6327) has been claimed to have many singular characteristics. To explain its unusually rounded and relatively weak emission line profiles, it has been propos…

astro-ph.SR201936 cited

The Magnetic Early B-type Stars II: stellar atmospheric parameters in the era of Gaia

M. E. Shultz, G. A. Wade, Th. Rivinius +6

Atmospheric parameters determined via spectral modelling are unavailable for many of the known magnetic early B-type stars. We utilized high-resolution spectra together with NLTE m…