232 citations · 1.9k across the 89 of their papers we have counts for
7 papers · 1 filter
The surface magnetic field and chemical abundance distributions of the B2V helium-strong star HD184927
I. Yakunin, G. Wade, D. Bohlender +8
A new time series of high-resolution Stokes I and V spectra of the magnetic B2V star HD 184927 has been obtained in the context of the Magnetism in Massive Stars (MiMeS) Large Prog…
Emission from the Centrifugal Magnetospheres of Magnetic B-type Stars
Matt Shultz, Gregg Wade, Thomas Rivinius +2
Approximately 10% of B-type stars possess strong magnetic fields, and of these, 25% host centrifugal magnetospheres (CMs) in which the radiative wind, magnetic field, and rotationa…
Discovery of a Centrifugal Magnetosphere Around the He-Strong Magnetic B1 Star ALS 3694
Matt Shultz, Gregg Wade, Thomas Rivinius +2
We report the results of 6 nights of Canada-France-Hawaii Telescope spectropolarimetric ESPaDOnS observations of the He-strong, magnetic B1 type star ALS 3694. The longitudinal mag…
CMa: An Extremely Slowly Rotating Magnetic B0.7 IV Star
Matt Shultz, Gregg Wade, Thomas Rivinius +4
We present our analysis of 6 years of ESPaDOnS spectropolarimetry of the magnetic Cep star CMa (B0.7 IV). This high-precision magnetometry is consistent with a rotational…
Plasma Leakage from the Centrifugal Magnetospheres of Magnetic B-Type Stars
Matt Shultz, Gregg Wade, Thomas Rivinius +3
Magnetic B-type stars are often host to Centrifugal Magnetospheres (CMs). Here we describe the results of a population study encompassing the full sample of known magnetic early B-…
Deep Photospheric Emission Lines as Probes for Pulsational Waves
Th. Rivinius, M. Shultz, G. A. Wade
Weak line emission originating in the photosphere is well known from O stars and widely used for luminosity classification. The physical origin of the line emission are NLTE effect…