Search Results - "ROEDERER, Ian U"
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Finding r-II Sibling Stars in the Milky Way with the Greedy Optimistic Clustering Algorithm
Published in The Astrophysical journal (01-03-2023)“…R -process enhanced stars with [Eu/Fe] ≥ +0.7 (so-called r -II stars) are believed to have formed in an extremely neutron-rich environment in which a rare…”
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THE DIVERSE ORIGINS OF NEUTRON-CAPTURE ELEMENTS IN THE METAL-POOR STAR HD 94028: POSSIBLE DETECTION OF PRODUCTS OF i-PROCESS NUCLEOSYNTHESIS
Published in The Astrophysical journal (10-04-2016)“…We present a detailed analysis of the composition and nucleosynthetic origins of the heavy elements in the metal-poor ([Fe/H] = −1.62 ± 0.09) star HD 94028…”
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High-resolution Optical Spectroscopy of Stars in the Sylgr Stellar Stream
Published in The Astrophysical journal (20-09-2019)“…We observe two metal-poor main-sequence stars that are members of the recently discovered Sylgr stellar stream. We present radial velocities, stellar…”
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The R-process Alliance: First Release from the Southern Search for R-process-enhanced Stars in the Galactic Halo
Published in The Astrophysical journal (10-05-2018)“…The recent detection of a binary neutron star merger and the clear evidence of the decay of radioactive material observed in this event have, after 60 years of…”
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A New Test of Copper and Zinc Abundances in Late-type Stars Using Ultraviolet Cu ii and Zn ii Lines
Published in The Astrophysical journal (10-04-2018)“…We present new abundances derived from Cu i , Cu ii , Zn i , and Zn ii lines in six warm (5766 ≤ ≤ 6427 K), metal-poor (−2.50 ≤ [Fe/H] ≤ −0.95) dwarf and…”
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The R-Process Alliance: First Magellan/MIKE Release from the Southern Search for R-process-enhanced Stars
Published in The Astrophysical journal (01-08-2020)“…Extensive progress has recently been made in our understanding of heavy-element production via the r -process in the universe, specifically with the first…”
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GERMANIUM, ARSENIC, AND SELENIUM ABUNDANCES IN METAL-POOR STARS
Published in The Astrophysical journal (01-09-2012)“…The elements germanium (Ge, Z = 32), arsenic (As, Z = 33), and selenium (Se, Z = 34) span the transition from charged-particle or explosive synthesis of the…”
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Evidence for an Aspherical Population III Supernova Explosion Inferred from the Hyper-metal-poor Star HE 1327–2326
Published in The Astrophysical journal (10-05-2019)“…We present observational evidence that an aspherical supernova explosion could have occurred in the first stars in the early universe. Our results are based on…”
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Detailed abundances of 15 stars in the metal-poor globular cluster NGC 4833
Published in Monthly notices of the Royal Astronomical Society (01-06-2015)“…We have observed 15 red giant stars in the relatively massive, metal-poor globular cluster NGC 4833 using the Magellan Inamori Kyocera Echelle spectrograph at…”
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R-process-rich Stellar Streams in the Milky Way
Published in The Astrophysical journal (01-05-2021)“…We present high-resolution Magellan/MIKE spectra of 22 bright (9 < V < 13.5) metal-poor stars (−3.18 < [Fe/H] < −1.37) in three different stellar streams, the…”
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HD 222925: A New Opportunity to Explore the Astrophysical and Nuclear Conditions of r-process Sites
Published in The Astrophysical journal (01-07-2023)“…With the most trans-iron elements detected of any star outside the solar system, HD 222925 represents the most complete chemical inventory among metal-poor…”
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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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The R-Process Alliance: Chemodynamically Tagged Groups of Halo r-process-enhanced Stars Reveal a Shared Chemical-evolution History
Published in The Astrophysical journal (01-02-2021)“…We derive dynamical parameters for a large sample of 446 r -process-enhanced (RPE) metal-poor stars in the halo and disk systems of the Milky Way, based on…”
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14
Iron and neutron-capture element abundance variations in the globular cluster M2 (NGC 7089)
Published in Monthly notices of the Royal Astronomical Society (11-07-2014)“…We present CN and CH indices and Ca ii triplet metallicities for 34 giant stars and chemical abundances for 33 elements in 14 giants in the globular cluster…”
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15
Metal Mixing in the r-process Enhanced Ultrafaint Dwarf Galaxy Reticulum II
Published in The Astronomical journal (01-03-2023)“…The ultrafaint dwarf galaxy Reticulum II was enriched by a single rare and prolific r -process event. The r -process content of Reticulum II thus provides a…”
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The R-Process Alliance: Chemodynamically Tagged Groups. II. An Extended Sample of Halo r-process-enhanced Stars
Published in The Astrophysical journal (01-01-2023)“…Orbital characteristics based on Gaia Early Data Release 3 astrometric parameters are analyzed for ∼1700 r -process-enhanced (RPE; [Eu/Fe] > +0.3) metal-poor…”
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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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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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The R-Process Alliance: 2MASS J22132050–5137385, the Star with the Highest-known r-process Enhancement at [Eu/Fe] = +2.45
Published in The Astrophysical journal (01-08-2024)“…We present stellar parameters and chemical abundances of 47 elements detected in the bright (V = 11.63) very metal-poor ([Fe/H] = −2.20 ± 0.12) star 2MASS…”
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Abundance Analysis of Stars at Large Radius in the Sextans Dwarf Spheroidal Galaxy
Published in The Astrophysical journal (01-09-2023)“…We present the stellar parameters and chemical abundances of 30 elements for five stars located at large radii (3.5–10.7 times the half-light radius) in the…”
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