CAN THE GROWTH OF DUST GRAINS IN LOW-METALLICITY STAR-FORMING CLOUDS AFFECT THE FORMATION OF METAL-POOR LOW-MASS STARS?

• 資料種別: 記事
• タイトル: CAN THE GROWTH OF DUST GRAINS IN LOW-METALLICITY STAR-FORMING CLOUDS AFFECT THE FORMATION OF METAL-POOR LOW-MASS STARS?
• 著者標目: Takaya Nozawa; Takashi Kozasa; Ken'ichi Nomoto
• 出版年月日等: 2012-08-23
• 出版年（W3CDTF）: 2012-08-23
• タイトル（掲載誌）: The Astrophysical Journal
• 巻号年月日等（掲載誌）: 756 2
• 掲載巻: 756
• 掲載号: 2
• 掲載ページ: L35-
• 掲載年月日（W3CDTF）: 2012-08-23
• ISSN（掲載誌）: 20418205; http://id.crossref.org/issn/0004637X
• 出版事項（掲載誌）: American Astronomical Society
• 件名標目: Space and Planetary Science; Astronomy and Astrophysics
• 対象利用者: 一般
• DOI: 10.1088/2041-8205/756/2/l35
• 作成日（W3CDTF）: 2012-08-23
• 参照: Gravitational instability in protostellar discs at low metallicities; https://cir.nii.ac.jp/crid/1360004234657996288; Supernova dust formation and the grain growth in the early universe: the critical metallicity for low-mass star formation; https://cir.nii.ac.jp/crid/1360285709635220480; THE ORIGIN OF THE MOST IRON-POOR STAR; https://cir.nii.ac.jp/crid/1360848659315026432; GROWTH OF DUST GRAINS IN A LOW-METALLICITY GAS AND ITS EFFECT ON THE CLOUD FRAGMENTATION; https://cir.nii.ac.jp/crid/1360848659396830592; Dust grain growth and the formation of the extremely primitive star SDSS J102915+172927; https://cir.nii.ac.jp/crid/1360848659588497664; Gravitational collapse and the thermal evolution of low-metallicity gas clouds in the early Universe; https://cir.nii.ac.jp/crid/1360848659590093312; Gravitational fragmentation of extremely metal-poor circumstellar discs; https://cir.nii.ac.jp/crid/1360857593709358464
• 参照: An extremely primitive star in the Galactic halo; https://cir.nii.ac.jp/crid/1360011144750125696; Evolution of interstellar dust and stardust in the solar neighbourhood; https://cir.nii.ac.jp/crid/1360011146503886976; Theory of Star Formation; https://cir.nii.ac.jp/crid/1360011146570668672; The first low-mass stars: critical metallicity or dust-to-gas ratio?; https://cir.nii.ac.jp/crid/1360565168155818240; The formation of the extremely primitive star SDSS J102915+172927 relies on dust; https://cir.nii.ac.jp/crid/1360565168254879744; Dust Destruction in the High‐Velocity Shocks Driven by Supernovae in the Early Universe; https://cir.nii.ac.jp/crid/1361137044208624000; Evolution of Dust in Primordial Supernova Remnants: Can Dust Grains Formed in the Ejecta Survive and Be Injected into the Early Interstellar Medium?; https://cir.nii.ac.jp/crid/1361137046261668224; Protostellar Collapse with Various Metallicities; https://cir.nii.ac.jp/crid/1361137046291433472; Effects of grain size distribution on the interstellar dust mass growth; https://cir.nii.ac.jp/crid/1361699994559379840; Fragmentation of star-forming clouds enriched with the first dust; https://cir.nii.ac.jp/crid/1361981469053890816; Abundances of the elements: Meteoritic and solar; https://cir.nii.ac.jp/crid/1361981470778238464; THE EFFECT OF DUST COOLING ON LOW-METALLICITY STAR-FORMING CLOUDS; https://cir.nii.ac.jp/crid/1362262943891599360; On the formation of very metal poor stars: the case of SDSS J1029151+172927; https://cir.nii.ac.jp/crid/1362825895038656384; Low-mass relics of early star formation; https://cir.nii.ac.jp/crid/1362825895284592256; Dust-cooling-induced Fragmentation of Low-Metallicity Clouds; https://cir.nii.ac.jp/crid/1362825896181017472; Thermal and Fragmentation Properties of Star‐forming Clouds in Low‐Metallicity Environments; https://cir.nii.ac.jp/crid/1363107369603131520; Dust in the Early Universe: Dust Formation in the Ejecta of Population III Supernovae; https://cir.nii.ac.jp/crid/1363107369697989632; Dust coagulation in star formation with different metallicities; https://cir.nii.ac.jp/crid/1363670319209634560
• 連携機関・データベース: 国立情報学研究所 : CiNii Research
• 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