The Hamburg/ESO R-process Enhanced Star survey (HERES)
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201424017/pdf
Reference147 articles.
1. Non-LTE sodium abundance in galactic thick- and thin-disk red giants
2. NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars
3. Non-LTE abundances of Mg and K in extremely metal-poor stars and the evolution of [O/Mg], [Na/Mg], [Al/Mg], and [K/Mg] in the Milky Way
4. Width cross-sections for collisional broadening of s–p and p–s transitions by atomic hydrogen
5. Spectroscopic Studies of Very Metal‐poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron‐Capture Elements
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1. The R-Process Alliance: 2MASS J22132050–5137385, the Star with the Highest-known r-process Enhancement at [Eu/Fe] = +2.45*;The Astrophysical Journal;2024-08-01
2. Detection of the Actinide Th in an r-process-enhanced Star with Accretion Origin;The Astrophysical Journal;2024-04-01
3. On the chemical composition of the evolved very bright metal‐poor star HD 1936;Astronomische Nachrichten;2024-02-28
4. SPLUS J142445.34–254247.1: An r-process–enhanced, Actinide-boost, Extremely Metal-poor Star Observed with GHOST;The Astrophysical Journal;2023-12-01
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