Astronomy:Heavy metal subdwarf

From HandWiki
Revision as of 16:28, 16 June 2021 by imported>NBrushPhys (correction)
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)

The heavy metal subdwarfs are a type of hot subdwarf star with high concentrations of heavy metals. The metals detected include germanium, strontium, yttrium, zirconium and lead. Known heavy metal subdwarfs include HE 2359-2844, LS IV-14 116, and HE 1256-2738.[1]

References

  1. ↑ "Astronomers Discover Two Heavy Metal Stars | Astronomy | Sci-News.com". 2 August 2013. http://www.sci-news.com/astronomy/science-heavy-metal-stars-01283.html. Retrieved 5 November 2016. 




Retrieved from "https://handwiki.org/wiki/index.php?title=Astronomy:Heavy_metal_subdwarf&oldid=473667"