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Metal abundances in hot white dwarfs with signatures of a superionized wind
About a dozen hot white dwarfs with effective temperatures T(eff) = 65 000 K – 120 000 K exhibit unusual absorption features in their optical spectra. These objects were tentatively identified as Rydberg lines of ultra-high excited metals in ionization stages v–x, indicating line formation in a dens...
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| Yayımlandı: | Astron Astrophys |
|---|---|
| Asıl Yazarlar: | , , |
| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
2018
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| Konular: | |
| Online Erişim: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6999747/ https://ncbi.nlm.nih.gov/pubmed/32020917 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1051/0004-6361/201731740 |
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