232 citations · 443 across the 9 of their papers we have counts for
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Magnetic field topology and chemical abundance distributions of the young, rapidly rotating chemically peculiar star HR5624
O. Kochukhov, J. Silvester, J. D. Bailey +2
The young, rapidly rotating Bp star HR5624 (HD133880) shows an unusually strong non-sinusoidal variability of its longitudinal magnetic field. This behaviour was previously interpr…
BD-19 5044L: discovery of a short-period SB2 system with a magnetic Bp primary in the open cluster IC 4725
J. D. Landstreet, O. Kochukhov, E. Alecian +5
Until recently almost nothing was known about the evolution of magnetic fields found in upper main sequence Ap/Bp stars during their long main sequence lifetime. We are thus studyi…
The MiMeS Survey of Magnetism in Massive Stars: Introduction and overview
G. A. Wade, C. Neiner, E. Alecian +47
The MiMeS project is a large-scale, high resolution, sensitive spectropolarimetric investigation of the magnetic properties of O and early B type stars. Initiated in 2008 and compl…
A Comprehensive Analysis of the Magnetic Standard Star HD 94660: Host of a Massive Compact Companion?
J. D. Bailey, J. Grunhut, J. D. Landstreet
Detailed information about the magnetic geometry, atmospheric abundances and radial velocity variations has been obtained for the magnetic standard star HD 94660 based on high-disp…
Measuring the surface magnetic fields of magnetic stars with unresolved Zeeman splitting
J. D. Bailey
High-dispersion, archival spectra of magnetic Ap stars with resolved Zeeman components in Stokes I are used to derive a simple relation that can be utilised to estimate the mean su…
Discovery of secular variations in the atmospheric abundances of magnetic Ap stars
J. D. Bailey, J. D. Landstreet, S. Bagnulo
The stars of the middle main sequence have relatively quiescent outer layers, and unusual chemical abundance patterns may develop in their atmospheres. The presence of chemical pec…
Abundances determined using Si II and Si III in B-type stars: evidence for stratification
Jeffrey D. Bailey, John D. Landstreet
It is becoming clear that determination of the abundance of Si using lines of Si II and Si III can lead to quite discordant results in mid to late B-type stars. The difference betw…
An Analysis of the Rapidly Rotating Bp Star HD 133880
J. D. Bailey, J. Grunhut, M. Shultz +8
HD 133880 is a rapidly rotating Bp star and host to one of the strongest magnetic fields of any Bp star. A member of the Upper Centaurus Lupus association, it is a star with a well…
Magnetic Field and Atmospheric Chemical Abundances of the Magnetic Ap Star HD 318107
J. D. Bailey, J. D. Landstreet, S. Bagnulo +5
New spectra have been obtained with the ESPaDOnS spectropolarimeter supplemented with unpolarised spectra from the ESO UVES, UVES-FLAMES, and HARPS spectrographs of the very peculi…