Spectrophotometric analysis of magnetic white dwarf: II. Helium-rich compositions
We present an analysis of all single white dwarf stars known to exhibit spectroscopic signatures of neutral helium line splitting due to the presence of a strong magnetic field. Using state-of-the-art models taking into account the effects of magnetic fields on the synthetic spectra, we determine ef...
Gespeichert in:
| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
April 2023
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2023, Jahrgang: 520, Heft: 4, Pages: 6135-6158 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stad197 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stad197 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/520/4/6135/6998574 
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| Verfasserangaben: | François Hardy, Patrick Dufour and Stefan Jordan |
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| 520 | |a We present an analysis of all single white dwarf stars known to exhibit spectroscopic signatures of neutral helium line splitting due to the presence of a strong magnetic field. Using state-of-the-art models taking into account the effects of magnetic fields on the synthetic spectra, we determine effective temperatures, surface gravities, and masses for the stars in our sample. ... | ||
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