Spectropolarimetric survey of hydrogen-rich white dwarf stars

A. Kawka*, S. Vennes, G. D. Schmidt, D. T. Wickramasinghe, R. Koch

*Corresponding author for this work

    Research output: Contribution to journalReview articlepeer-review

    149 Citations (Scopus)

    Abstract

    We have conducted a survey of 61 southern white dwarfs searching for magnetic fields using Zeeman spectropolarimetry. Our objective is to obtain a magnetic field distribution for these objects and, in particular, to find white dwarfs with weak fields. We found one possible candidate (WD 0310-688) that may have a weak magnetic field of -6.1 ±2.2 kG. Next, we determine the fraction and distribution of magnetic white dwarfs in the solar neighborhood and investigate the probability of finding more of these objects based on the current incidence of magnetism in white dwarfs within 20 pc of the Sun. We have also analyzed the spectra of the white dwarfs to obtain effective temperatures and surface gravities.

    Original languageEnglish
    Pages (from-to)499-520
    Number of pages22
    JournalAstrophysical Journal
    Volume654
    Issue number1 I
    DOIs
    Publication statusPublished - 1 Jan 2007

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