What it is
In this study, we report the discovery of WD J132800.85–145019.95, a new gas-disc system that exhibits quadruple-peaked instead of double-peaked line profiles. These emission lines originate from two separate gaseous rings extending from 0.14 R ⊙ to 0.34 R ⊙ and from 0.54 R ⊙ to 1.93 R ⊙.
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Filed underStellar, planetary, and galactic studies, Astro and Planetary Science, Astrophysics and Star Formation Studies