Phase-Resolved Spectroscopy of the Polar V379 Vir with a Brown Dwarf
Abstract
The polar V379 Vir is a well-known magnetic cataclysmic variable with a brown dwarf donor. Despite numerous studies of this system across various spectral ranges, a detailed investigation of the orbital variability of its optical spectra has not been carried out. In this work, we present an analysis of spectroscopic observations of V379 Vir obtained with the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. The orbital variability of the H $$\alpha$$ emission indicates that the line is most likely formed in the accretion stream near the Lagrangian point $$L_{1}$$ , rather than on the donor’s surface, as previously assumed. The analysis of the rotational variability of the Zeeman splitting of hydrogen lines reveals a complex magnetic field topology of the white dwarf, which differs from a simple dipole configuration.
Fields of Study & Subjects
Astrophysical Phenomena and Observations
Astronomy and Astrophysical Research
Stellar
planetary
and galactic studies
Publication details
- Journal / source
- Astrophysical Bulletin
- Publisher
- Pleiades Publishing Ltd
- Volume
- 81
- Issue
- 1
- Pages
- 44–53
- Publication date
- 1 March 2026
- Language
- EN