Search Results - "Hartog, Elizabeth A Den"
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Detailed Iron-peak Element Abundances in Three Very Metal-poor Stars
Published in The Astrophysical journal (20-02-2020)“…We have obtained new detailed abundances of the Fe-group elements Sc through Zn ( Z = 21–30) in three very metal-poor ([Fe/H] ≈ −3) stars: BD+03 o 740, BD−13…”
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IRON-GROUP ABUNDANCES IN THE METAL-POOR MAIN-SEQUENCE TURNOFF STAR HD 84937
Published in The Astrophysical journal (20-01-2016)“…ABSTRACT We have derived new, very accurate abundances of the Fe-group elements Sc through Zn (Z = 21−30) in the bright main-sequence turnoff star HD 84937…”
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The R-process Alliance: A Nearly Complete R-process Abundance Template Derived from Ultraviolet Spectroscopy of the R-process-enhanced Metal-poor Star HD 222925
Published in The Astrophysical journal. Supplement series (01-06-2022)“…We present a nearly complete rapid neutron-capture process ( r -process) chemical inventory of the metal-poor ([Fe/H] = −1.46 ± 0.10) r -process-enhanced…”
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Iron-peak Element Abundances in Warm Very Metal-poor Stars
Published in The Astrophysical journal (01-08-2023)“…We have derived new detailed abundances of Mg, Ca, and the Fe-group elements Sc through Zn ( Z = 21−30) for 37 main-sequence turnoff very metal-poor stars…”
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The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks
Published in The Astrophysical journal (01-09-2022)“…We present new observational benchmarks of rapid neutron-capture process ( r -process) nucleosynthesis for elements at and between the first ( A ∼ 80) and…”
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Atomic data for stellar spectroscopy: recent successes and remaining needs
Published in Physica scripta (01-11-2014)“…Stellar chemical composition analyses provide vital insights into galactic nucleosynthesis. Atomic line data are critical inputs to stellar abundance…”
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Iron-Peak Element Abundances in Warm Very Metal-Poor Stars
Published 14-04-2023“…We have derived new detailed abundances of Mg, Ca, and the Fe-group elements Sc through Zn (Z = 21-30) for 37 main sequence turnoff very metal-poor stars…”
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The R-Process Alliance: A Nearly Complete R-Process Abundance Template Derived from Ultraviolet Spectroscopy of the R-Process-Enhanced Metal-Poor Star HD 222925
Published 18-05-2022“…We present a nearly complete rapid neutron-capture process (r-process) chemical inventory of the metal-poor ([Fe/H] = -1.46 +/- 0.10) r-process-enhanced…”
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linemake: An Atomic and Molecular Line List Generator
Published 16-04-2021“…Research Notes of the AAS, 2021, 5, 92 In this research note, we present linemake, an open-source atomic and molecular line list generator. Rather than a…”
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The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks
Published 27-10-2022“…Astrophysical Journal Vol. 936, p. 84 (2022) We present new observational benchmarks of rapid neutron-capture process (r-process) nucleosynthesis for elements…”
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Detailed Iron-Peak Element Abundances in Three Very Metal-Poor Stars
Published 02-01-2020“…We have obtained new detailed abundances of the Fe-group elements Sc through Zn (Z=21-30) in three very metal-poor ([Fe/H] $\approx -3$) stars: BD 03 740, BD…”
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The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks Based on archival observations made with the NASA/ESA Hubble Space Telescope (program GO-7348, program GO-8342, program GO-9455, program GO-14161, and program GO-14672) and observations collected from the Keck Observatory Archive (program U25H)
Published in The Astrophysical journal (01-09-2022)Get full text
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The R-process Alliance: A Nearly Complete R-process Abundance Template Derived from Ultraviolet Spectroscopy of the R-process-enhanced Metal-poor Star HD 222925 Based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract NAS 5-26555. These observations are primarily associated with program GO-15657. Data from programs GO-7348, GO-819
Published in The Astrophysical journal. Supplement series (17-06-2022)Get full text
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Detailed Iron-peak Element Abundances in Three Very Metal-poor Stars Based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute (STScI), which is operated by the Association of Universities for Research in Astronomy, Inc. (AURA) under NASA contract NAS 5-26555. These observations are associated with program GO-14232. Some data presented in this paper were obtained from the Barbara A. Mikulski Archive for Space Telescopes (MAST). These d
Published in The Astrophysical journal (19-02-2020)“…We have obtained new detailed abundances of the Fe-group elements Sc through Zn (Z = 21-30) in three very metal-poor ([Fe/H] −3) stars: BD+03o740, BD−13o3442,…”
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Iron-Group Abundances in the Metal-Poor Main Sequence Turnoff Star HD~84937
Published 18-11-2015“…We have derived new very accurate abundances of the Fe-group elements Sc through Zn (Z = 21-30) in the bright main-sequence turnoff star HD 84937, based on…”
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New Rare Earth Element Abundance Distributions for the Sun and Five r-Process-Rich Very Metal-Poor Stars
Published 09-03-2009“…We have derived new abundances of the rare-earth elements Pr, Dy, Tm, Yb, and Lu for the solar photosphere and for five very metal-poor, neutron-capture…”
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