What it is
In this study, we report the discovery of a white dwarf accreting material that is unlike any Solar System object. The atmosphere of HS 0209+0832 is strongly enriched in trans-iron elements including zinc, copper and niobium but depleted in the canonical rock-forming elements silicon and iron.
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Filed underStellar, planetary, and galactic studies, Astro and Planetary Science, Astrophysical Phenomena and Observations