Identifiers
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name variant
(3) IPNAS
0.60 · backfill
Papers (10)
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Stellar 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
astro-ph.SR · 2017 · author #16
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Stellar laboratories. VIII. New Zr IV - VII, Xe IV - V, and Xe VII oscillator strengths and the Al, Zr, and Xe abundances in the hot white dwarfs G191-B2B and RE0503-289
physics.atom-ph · 2016 · author #17
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Stellar laboratories. VII. New Kr IV - VII oscillator strengths and an improved spectral analysis of the hot, hydrogen-deficient DO-type white dwarf RE0503-289
astro-ph.SR · 2016 · author #16
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Stellar laboratories. VI. New Mo IV - VII oscillator strengths and the molybdenum abundance in the hot white dwarfs G191-B2B and RE0503-289
astro-ph.SR · 2015 · author #15
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Stellar laboratories. V. The Xe VI ultraviolet spectrum and the xenon abundance in the hot DO-type white dwarf RE0503-289
astro-ph.SR · 2015 · author #14
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Stellar laboratories IV. New Ga IV, Ga V, and Ga VI oscillator strengths and the gallium abundance in the hot white dwarfs G191-B2B and RE0503-289
astro-ph.SR · 2015 · author #13
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Stellar laboratories III. New Ba V, Ba VI, and Ba VII oscillator strengths and the barium abundance in the hot white dwarfs G191-B2B and RE0503-289
astro-ph.SR · 2014 · author #13
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Stellar laboratories II. New Zn IV and Zn V oscillator strengths and their validation in the hot white dwarfs G191-B2B and RE0503-289
astro-ph.SR · 2014 · author #13
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Stellar laboratories: new Ge V and Ge VI oscillator strengths and their validation in the hot white dwarf RE 0503-289
astro-ph.SR · 2012 · author #18
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Cerium: the lithium substitute in post-AGB stars
astro-ph · 2002 · author #10
Mentions
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1504.01991
#14 · backfill · confidence 0.70
(3) IPNAS
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1501.07751
#13 · backfill · confidence 0.70
(3) IPNAS
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1404.6094
#13 · backfill · confidence 0.70
(3) IPNAS
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1403.2183
#13 · backfill · confidence 0.70
(3) IPNAS
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1209.0642
#18 · backfill · confidence 0.70
(3) IPNAS