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20172020
most citedStellar laboratories. IX. New Se V, Sr IV - VII, Te VI, and I VI oscillator strengths and the Se, Sr, Te, and I abundances in the hot white dwarfs G191-B2B and RE 0503-289

30 citations · 70 across the 3 of their papers we have counts for

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Showing 2018Show all

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astro-ph.SR2018★ 25 cited

First detection of bromine and antimony in hot stars

K. Werner, T. Rauch, M. Knoerzer +1

Bromine (atomic number Z=35) and antimony (Z=51) are extremely difficult to detect in stars. In very few instances, weak and mostly uncertain identifications of Br I, Br II, and Sb…