Abstract
Our ongoing spectroscopic survey of high proper motion stars is a rich source of new magnetic white dwarfs. We present a few examples among cool white dwarfs showing the effect of field strength and geometry on the observed optical spectrum. Modelling of hydrogen and heavy element spectral lines reveals a range of uniform or markedly offset dipole fields in these objects.
| Original language | English |
|---|---|
| Pages (from-to) | 307-311 |
| Number of pages | 5 |
| Journal | Contributions of the Astronomical Observatory Skalnate Pleso |
| Volume | 48 |
| Issue number | 1 |
| Publication status | Published - 2018 |