Formation of Carbon-enhanced Metal-poor Stars As a Consequence of Inhomogeneous Metal Mixing

• 資料種別: 記事
• タイトル: Formation of Carbon-enhanced Metal-poor Stars As a Consequence of Inhomogeneous Metal Mixing
• 著者標目: Tilman Hartwig; Naoki Yoshida
• 出版年月日等: 2019-01-01
• 出版年（W3CDTF）: 2019-01-01
• タイトル（掲載誌）: The Astrophysical Journal Letters
• 巻号年月日等（掲載誌）: 870 1
• 掲載巻: 870
• 掲載号: 1
• 掲載ページ: L3-
• 掲載年月日（W3CDTF）: 2019-01-01
• ISSN（掲載誌）: 20418205
• 出版事項（掲載誌）: American Astronomical Society
• 件名標目: Cosmology and Nongalactic Astrophysics (astro-ph.CO); Astrophysics of Galaxies (astro-ph.GA); FOS: Physical sciences; Astrophysics - Astrophysics of Galaxies; Astrophysics - Cosmology and Nongalactic Astrophysics
• 対象利用者: 一般
• DOI: 10.3847/2041-8213/aaf866; https://doi.org/10.3847/2041-8213/aaf866; 10.48550/arxiv.1812.01820; https://doi.org/10.48550/arxiv.1812.01820
• 作成日（W3CDTF）: 2019-01-03
• オンライン閲覧公開範囲: インターネット公開
• 著作権情報: https://iopscience.iop.org/page/copyright; https://iopscience.iop.org/info/page/text-and-data-mining
• 関連情報（URI）: https://iopscience.iop.org/article/10.3847/2041-8213/aaf866/pdf; https://iopscience.iop.org/article/10.3847/2041-8213/aaf866
• 参照: Photoevaporation of Minihalos During Cosmic Reionization: Primordial and Metal-enriched Halos; https://cir.nii.ac.jp/crid/1360009142484460416; Origin of metals in old Milky Way halo stars based on GALAH and Gaia; https://cir.nii.ac.jp/crid/1360013168722356096; Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances; https://cir.nii.ac.jp/crid/1360017279841206784; Public Release of A-SLOTH: Ancient Stars and Local Observables by Tracing Halos; https://cir.nii.ac.jp/crid/1360298757440952960; Chemodynamically Tagged Groups of CEMP Stars in the Halo of the Milky Way. I. Untangling the Origins of CEMP-s and CEMP-no Stars; https://cir.nii.ac.jp/crid/1360302864786033280; Implications of Inhomogeneous Metal Mixing for Stellar Archaeology; https://cir.nii.ac.jp/crid/1360572092843276928; Does the structure of Population III supernova ejecta affect the elemental abundance of extremely metal-poor stars?; https://cir.nii.ac.jp/crid/1360853567705804416; Chemical abundances of field halo stars - Implications for the building blocks of the Milky Way; https://cir.nii.ac.jp/crid/1361131417874110592
• 参照: CARBON-ENHANCED METAL-POOR STAR FREQUENCIES IN THE GALAXY: CORRECTIONS FOR THE EFFECT OF EVOLUTIONARY STATUS ON CARBON ABUNDANCES; https://cir.nii.ac.jp/crid/1360011144336944896; THE NUCLEOSYNTHETIC IMPRINT OF 15–40<i>M</i>_☉PRIMORDIAL SUPERNOVAE ON METAL-POOR STARS; https://cir.nii.ac.jp/crid/1360011145196644864; Abundance anomalies in metal-poor stars from Population III supernova ejecta hydrodynamics; https://cir.nii.ac.jp/crid/1360011145532451712; The Chemical Composition of the Sun; https://cir.nii.ac.jp/crid/1360011145591342208; The formation of direct collapse black holes under the influence of streaming velocities; https://cir.nii.ac.jp/crid/1360011145593054848; FAINT POPULATION III SUPERNOVAE AS THE ORIGIN OF THE MOST IRON-POOR STARS; https://cir.nii.ac.jp/crid/1360283692449089024; Limits on Population III star formation with the most iron-poor stars; https://cir.nii.ac.jp/crid/1360283692576641664; Descendants of the first stars: the distinct chemical signature of second-generation stars; https://cir.nii.ac.jp/crid/1360285709638344448; CARBON-ENHANCED METAL-POOR STARS IN SDSS/SEGUE. I. CARBON ABUNDANCE ESTIMATION AND FREQUENCY OF CEMP STARS; https://cir.nii.ac.jp/crid/1360292621340427904; Classification of extremely metal-poor stars: absent region in <i>A</i>(C)–[Fe/H] plane and the role of dust cooling; https://cir.nii.ac.jp/crid/1360565167554923264; The first low-mass stars: critical metallicity or dust-to-gas ratio?; https://cir.nii.ac.jp/crid/1360565168155818240; Fingerprint of the first stars: multi-enriched extremely metal-poor stars in the TOPoS survey; https://cir.nii.ac.jp/crid/1360567184615687680; Origins of carbon-enhanced metal-poor stars; https://cir.nii.ac.jp/crid/1360574095206830336; Metal-poor star formation triggered by the feedback effects from Pop III stars; https://cir.nii.ac.jp/crid/1360846642530692224; Nucleosynthesis in Stars and the Chemical Enrichment of Galaxies; https://cir.nii.ac.jp/crid/1360846643567380224; Preserving chemical signatures of primordial star formation in the first low-mass stars; https://cir.nii.ac.jp/crid/1360855568500764160; Three-dimensional neutrino-driven supernovae: Neutron star kicks, spins, and asymmetric ejection of nucleosynthesis products; https://cir.nii.ac.jp/crid/1360855571215992320; Carbon‐enhanced Metal‐poor Stars. I. Chemical Compositions of 26 Stars; https://cir.nii.ac.jp/crid/1361137045188849024; The First Supernova Explosions: Energetics, Feedback, and Chemical Enrichment; https://cir.nii.ac.jp/crid/1361137045455015040; Protostellar Collapse with Various Metallicities; https://cir.nii.ac.jp/crid/1361137046291433472; ASPHERICAL PROPERTIES OF HYDRODYNAMICS AND NUCLEOSYNTHESIS IN JET-INDUCED SUPERNOVAE; https://cir.nii.ac.jp/crid/1361418519369861760; The Discovery and Analysis of Very Metal-Poor Stars in the Galaxy; https://cir.nii.ac.jp/crid/1361418520561297408; THE EARLY EVOLUTION OF PRIMORDIAL PAIR-INSTABILITY SUPERNOVAE; https://cir.nii.ac.jp/crid/1361418520692142336; JINAbase—A Database for Chemical Abundances of Metal-poor Stars; https://cir.nii.ac.jp/crid/1361418521303621120; Metal transport and chemical heterogeneity in early star forming systems; https://cir.nii.ac.jp/crid/1361699993465461120; The First Chemical Enrichment in the Universe and the Formation of Hyper Metal-Poor Stars; https://cir.nii.ac.jp/crid/1361699994442476800; MIXING OF CLUMPY SUPERNOVA EJECTA INTO MOLECULAR CLOUDS; https://cir.nii.ac.jp/crid/1361981469391438208; OBSERVATIONAL CONSTRAINTS ON FIRST-STAR NUCLEOSYNTHESIS. I. EVIDENCE FOR MULTIPLE PROGENITORS OF CEMP-NO STARS; https://cir.nii.ac.jp/crid/1361981469571472768; Stellar Abundances for the Galactic Archeology (SAGA) Database — Compilation of the Characteristics of Known Extremely Metal-Poor Stars; https://cir.nii.ac.jp/crid/1361981470775591552; Supernova Nucleosynthesis in Population III 13–50<i>M</i>_⊙Stars and Abundance Patterns of Extremely Metal‐poor Stars; https://cir.nii.ac.jp/crid/1362262944310666496; FOLLOWING THE COSMIC EVOLUTION OF PRISTINE GAS. I. IMPLICATIONS FOR MILKY WAY HALO STARS; https://cir.nii.ac.jp/crid/1362262945041923968; THE MOST METAL-POOR STARS. III. THE METALLICITY DISTRIBUTION FUNCTION AND CARBON-ENHANCED METAL-POOR FRACTION, ,; https://cir.nii.ac.jp/crid/1362262946166779904; Photodissociation Feedback of Population III Stars onto Neighboring Prestellar Cores; https://cir.nii.ac.jp/crid/1362544419284867840; Explosive Nucleosynthesis in Aspherical Hypernova Explosions and Late‐Time Spectra of SN 1998bw; https://cir.nii.ac.jp/crid/1362825893961522944; The Binary Frequency Among Carbon‐enhanced,<i>s</i>‐Process–rich, Metal‐poor Stars; https://cir.nii.ac.jp/crid/1363107368350433792; Near-Field Cosmology with Extremely Metal-Poor Stars; https://cir.nii.ac.jp/crid/1363107369136608384; Thermal and Fragmentation Properties of Star‐forming Clouds in Low‐Metallicity Environments; https://cir.nii.ac.jp/crid/1363107369603131520; Generic Spectrum and Ionization Efficiency of a Heavy Initial Mass Function for the First Stars; https://cir.nii.ac.jp/crid/1363670318508402688; The formation of the first low-mass stars from gas with low carbon and oxygen abundances; https://cir.nii.ac.jp/crid/1363670319135982976; Forming the First Stars in the Universe: The Fragmentation of Primordial Gas; https://cir.nii.ac.jp/crid/1363951793226494336; The first Population II stars formed in externally enriched mini-haloes; https://cir.nii.ac.jp/crid/1364233268446285056; Chemical Abundance Analysis of the Extremely Metal‐poor Star HE 1300+0157; https://cir.nii.ac.jp/crid/1364233268682774144; Recovery from Population III supernova explosions and the onset of second-generation star formation; https://cir.nii.ac.jp/crid/1364233269887004928; A search for stars of very low metal abundance. II; https://cir.nii.ac.jp/crid/1364233270676105344; On the photodissociation of H2 by the first stars; https://cir.nii.ac.jp/crid/1364233270894991488
• 連携機関・データベース: 国立情報学研究所 : CiNii Research; https://cir.nii.ac.jp/
• 提供元機関・データベース: Crossref; https://www.crossref.org; 科学研究費助成事業データベース; https://kaken.nii.ac.jp/ja

• 要約等: <jats:title>Abstract</jats:title> <jats:p>We present a novel scenario for the formation of carbon-enhanced metal-poor (CEMP) stars. Car...