# A new weak-field magnetic DA white dwarf in the local 20 pc volume. The frequency of magnetic fields in DA stars

## TL;DR

This paper reports the discovery of a weak-field magnetic white dwarf within 20 parsecs of the Sun and explores the prevalence of magnetic fields among nearby DA white dwarfs, finding about 20% are magnetic.

## Contribution

The paper presents the first detection of a weak magnetic field in a nearby DA white dwarf and estimates the magnetic fraction among local DA WDs.

## Key findings

- Approximately 20% of local DA white dwarfs have magnetic fields.
- Most magnetic DA WDs have fields weaker than 1 MG.
- No evidence of magnetic field decay over several billion years.

## Abstract

We report the discovery of a new magnetic DA white dwarf (WD), WD0011-721, which is located within the very important 20pc volume-limited sample of the closest WDs to the Sun. This star has a mean field modulus <|B|> of 343 kG, and from the polarisation signal we deduce a line-of-sight field component of 75 kG. The magnetic field is sufficiently weak to have escaped detection in classification spectra. We then present a preliminary exploration of the data concerning the frequency of such fields among WDs with hydrogen-rich atmospheres (DA stars). We find that 20 +- 5% of the DA WDs in this volume have magnetic fields, mostly weaker than 1 MG. Unlike the slow field decay found among the magnetic Bp stars of the upper main sequence, the WDs in this sample show no evidence of magnetic field or flux changes over several Gyr.