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Magnetic properties of intermediate-mass stars
Magnetic fields play an important role in producing and modifying the
photospheric chemical peculiarities of intermediate-mass main sequence stars.
This article discusses the basic theory and methods of measurement used to
detect and characterise stellar magnetic fields, and reviews our current
knowledge of selected characteristics of magnetic fields in intermediate-mass
stars.Comment: v2: Add comment paper source: To appear in proceedings of "Element
stratification in stars", held at Chateau de Mons, Franc
Stokes IQUV mapping of CVn & other Ap stars using ESPaDOnS and NARVAL
New spectral line polarisation observations of 7 bright Ap stars have been
obtained with the ESPaDOnS and Narval high resolution spectropolarimeters
(Silvester et al. 2012). The aim of this data set is produce a series of
surface magnetic field and surface chemistry maps for these Ap stars. We
present new magnetic maps for the Ap star CVn using these new data
and the MDI inversion code INVERS10. CVn is the first Ap star to be
observed during two separate epochs using high resolution phase resolved
spectropolarimetric observations and as such allows us an insight into
how stable the surface magnetic structure is over a decade timescale. We show
that the new maps give a magnetic field structure consistent with the previous
maps obtained by Kochukhov and Wade (2010) from lower quality MuSiCoS spectra
taken a decade ago and that the field topology cannot be described by a dipolar
or quadrupolar field.Comment: 6 pages, 3 figures. Proceedings of New advances in stellar physics:
from microscopic to macroscopic processes (Roscoff 2013
The magnetic field topology and chemical abundance distributions of the Ap star HD 32633
Previous observations of the Ap star HD 32633 indicated that its magnetic
field was unusually complex in nature and could not be characterised by a
simple dipolar structure. Here we derive magnetic field maps and chemical
abundance distributions for this star using full Stokes vector (Stokes )
high-resolution observations obtained with the ESPaDOnS and Narval
spectropolarimeters. Our maps, produced using the Invers10 magnetic Doppler
imaging (MDI) code, show that HD 32633 has a strong magnetic field which
features two large regions of opposite polarity but deviates significantly from
a pure dipole field. We use a spherical harmonic expansion to characterise the
magnetic field and find that the harmonic energy is predominately in the
and poloidal modes with a small toroidal component. At the
same time, we demonstrate that the observed Stokes parameter profiles of HD
32633 cannot be fully described by either a dipolar or dipolar plus quadrupolar
field geometry. We compare the magnetic field topology of HD 32633 with other
early-type stars for which MDI analyses have been performed, supporting a trend
of increasing field complexity with stellar mass. We then compare the magnetic
field topology of HD 32633 with derived chemical abundance maps for the
elements Mg, Si, Ti, Cr, Fe, Ni and Nd. We find that the iron-peak elements
show similar distributions, but we are unable to find a clear correlation
between the location of local chemical enhancements or depletions and the
magnetic field structure.Comment: 15 pages, 11 figures, accepted for publication in MNRA
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