Search Results - "Frebel, Anna"
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CHEMICAL SIGNATURES OF THE FIRST GALAXIES: CRITERIA FOR ONE-SHOT ENRICHMENT
Published in The Astrophysical journal (10-11-2012)“…We utilize metal-poor stars in the local, ultra-faint dwarf galaxies (UFDs; L sub(tot) [< or =, slant] 10 super(5) L sub([middot in circle])) to empirically…”
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R-process enrichment from a single event in an ancient dwarf galaxy
Published in Nature (London) (31-03-2016)“…It has long been debated whether elements heavier than zinc are formed continually, for example in core-collapse supernovae, or in rare events, such as neutron…”
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From Actinides to Zinc: Using the Full Abundance Pattern of the Brightest Star in Reticulum II to Distinguish between Different r-process Sites
Published in The Astrophysical journal (01-04-2018)“…Abstract The ultra-faint dwarf galaxy Reticulum II was enriched by a rare and prolific r -process event, such as a neutron star merger (NSM). To investigate…”
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COMPLETE ELEMENT ABUNDANCES OF NINE STARS IN THE r-PROCESS GALAXY RETICULUM II
Published in The Astrophysical journal (20-10-2016)“…ABSTRACT We present chemical abundances derived from high-resolution Magellan /Magellan Inamori Kyocera Echelle spectra of the nine brightest known red giant…”
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Ultra-metal-poor Stars: Spectroscopic Determination of Stellar Atmospheric Parameters Using Iron Non-LTE Line Abundances
Published in The Astrophysical journal (01-10-2017)“…We present new ultra-metal-poor stars parameters with [Fe/H] < −4.0 based on line-by-line non-local thermodynamic equilibrium (NLTE) abundances using an…”
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CARBON-ENHANCED METAL-POOR STAR FREQUENCIES IN THE GALAXY: CORRECTIONS FOR THE EFFECT OF EVOLUTIONARY STATUS ON CARBON ABUNDANCES
Published in The Astrophysical journal (10-12-2014)“…We revisit the observed frequencies of carbon-enhanced metal-poor (CEMP) stars as a function of the metallicity in the Galaxy, using data from the literature…”
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Preserving chemical signatures of primordial star formation in the first low-mass stars
Published in Monthly notices of the Royal Astronomical Society (21-11-2015)“…We model early star-forming regions and their chemical enrichment by Population III (Pop III) supernovae with nucleosynthetic yields featuring high [C/Fe]…”
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Chemical Abundances in the Ultra-faint Dwarf Galaxies Grus I and Triangulum II: Neutron-capture Elements as a Defining Feature of the Faintest Dwarfs
Published in The Astrophysical journal (10-01-2019)“…Abstract We present high-resolution spectroscopy of four stars in two candidate ultra-faint dwarf galaxies (UFDs), Grus I (Gru I) and Triangulum II (Tri II)…”
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The predicted luminous satellite populations around SMC- and LMC-mass galaxies – a missing satellite problem around the LMC?
Published in Monthly notices of the Royal Astronomical Society (21-11-2017)“…Abstract Recent discovery of many dwarf satellite galaxies in the direction of the Small and Large Magellanic Clouds (SMC and LMC) provokes questions of their…”
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HIGH-RESOLUTION SPECTROSCOPY OF EXTREMELY METAL-POOR STARS IN THE LEAST EVOLVED GALAXIES: BOÖTES II
Published in The Astrophysical journal (20-01-2016)“…ABSTRACT We present high-resolution Magellan /MIKE spectra of the four brightest confirmed red giant stars in the ultra-faint dwarf galaxy Boötes II (Boo II)…”
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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)“…Abstract 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…”
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Chemical Abundances of New Member Stars in the Tucana II Dwarf Galaxy
Published in The Astrophysical journal (10-04-2018)“…Abstract We present chemical abundance measurements for seven stars with metallicities ranging from Fe/H] = −3.3 to [Fe/H] = −2.4 in the Tucana II ultra-faint…”
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Collapsar R-process Yields Can Reproduce [Eu/Fe] Abundance Scatter in Metal-poor Stars
Published in The Astrophysical journal (01-07-2021)“…Abstract It is unclear if neutron star mergers can explain the observed r -process abundances of metal-poor stars. Collapsars, defined here as rotating massive…”
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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)“…Abstract Extensive progress has recently been made in our understanding of heavy-element production via the r -process in the universe, specifically with 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)“…Abstract We present observational evidence that an aspherical supernova explosion could have occurred in the first stars in the early universe. Our results are…”
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THE CATERPILLAR PROJECT: A LARGE SUITE OF MILKY WAY SIZED HALOS
Published in The Astrophysical journal (10-02-2016)“…ABSTRACT We present the largest number of Milky Way sized dark matter halos simulated at very high mass (∼104 /particle) and temporal resolution (5…”
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Predicting the locations of possible long-lived low-mass first stars: importance of satellite dwarf galaxies
Published in Monthly notices of the Royal Astronomical Society (01-02-2018)“…Abstract The search for metal-free stars has so far been unsuccessful, proving that if there are surviving stars from the first generation, they are rare, they…”
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Descendants of the first stars: the distinct chemical signature of second-generation stars
Published in Monthly notices of the Royal Astronomical Society (01-08-2018)“…ABSTRACT Extremely metal-poor (EMP) stars in the Milky Way (MW) allow us to infer the properties of their progenitors by comparing their chemical composition…”
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The R-Process Alliance: First Release from the Northern Search for r-process-enhanced Metal-poor Stars in the Galactic Halo
Published in The Astrophysical journal (01-12-2018)“…This paper presents the detailed abundances and r-process classifications of 126 newly identified metal-poor stars as part of an ongoing collaboration, the…”
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SEGUE 1-A COMPRESSED STAR FORMATION HISTORY BEFORE REIONIZATION
Published in The Astrophysical journal (10-02-2016)“…ABSTRACT Segue 1 is the current best candidate for a "first galaxy," a system that experienced only a single, short burst of star formation and has since…”
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