Issue |
A&A
Volume 462, Number 3, February II 2007
|
|
---|---|---|
Page(s) | 1097 - 1101 | |
Section | Stellar atmospheres | |
DOI | https://doi.org/10.1051/0004-6361:20066163 | |
Published online | 21 November 2006 |
The fraction of DA white dwarfs with kilo-Gauss magnetic fields *,**
1
Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr. 12-14, 69120 Heidelberg, Germany e-mail: jordan@ari.uni-heidelberg.de
2
Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany e-mail: [aznar;solanki]@linmpi.mpg.de
3
Centre for Astrophysics Research, University of Hertfordshire, Hatfield AL10 9AB, UK e-mail: rn@star.herts.ac.uk
4
Institut für Astronomie, ETH Zürich, 8092 Zürich, Switzerland e-mail: schmid@astro.phys.ethz.ch
Received:
2
August
2006
Accepted:
12
October
2006
Context.Weak magnetic fields have been searched for on only a small number of white dwarfs. Current estimates find that about 10% of all white dwarfs have fields in excess of 1 MG; according to previous studies this number increases up to about 25% in the kG regime.
Aims.Our aim is to improve on these statistics by a new sample of ten white dwarfs in order to determine the ratio of magnetic to field-free white dwarfs.
Methods.Mean longitudinal magnetic fields strengths were determined by means of high-precision circular polarimetry of Hβ and Hγ with the FORS1 spectrograph of the VLT “Kueyen” 8 m telescope.
Results.In one of our objects (LTT 7987), we detected a statistically
significant (97% confidence level) longitudinal magnetic
field varying between () kG and (
) kG.
This would be the weakest magnetic field ever found in a white dwarf,
but systematic errors cannot completely
be ruled out at this level of accuracy. We also observed the sdO star EC 11481-2303 but could
not detect a magnetic field.
Conclusions. VLT observations with uncertainties typically of 1000 G or less suggest that 15-20% of WDs have kG fields. Together with previous investigations, the fraction of kG magnetic fields in white dwarfs amounts to about 11-15%, which is close to the current estimations for highly magnetic white dwarfs (>1 MG).
Key words: stars: white dwarfs / stars: magnetic fields
© ESO, 2007
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.