標(biāo)題: Titlebook: Understanding the Enrichment of Heavy Elements by the Chemodynamical Evolution Models of Dwarf Galax; Yutaka Hirai Book 2019 Springer Natu [打印本頁(yè)] 作者: 母牛膽小鬼 時(shí)間: 2025-3-21 17:18
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書目名稱Understanding the Enrichment of Heavy Elements by the Chemodynamical Evolution Models of Dwarf Galax讀者反饋
書目名稱Understanding the Enrichment of Heavy Elements by the Chemodynamical Evolution Models of Dwarf Galax讀者反饋學(xué)科排名
作者: esculent 時(shí)間: 2025-3-21 23:41 作者: 懲罰 時(shí)間: 2025-3-22 01:42 作者: Affectation 時(shí)間: 2025-3-22 04:55
Yutaka Hiraias unworthy of the author of the Tractatus and the I nvestiga- tions. This is unfortunate, I believe, and not at all fair, for these remarks are not only enjoyable reading, as even the harshest critics have con- ceded, but also a rich and genuine source of insight into the nature of mathematics. It 作者: CANDY 時(shí)間: 2025-3-22 11:33
Yutaka Hiraimothers of those children.Discusses the demographic of the c.This pioneering volume brings a rarely-studied population--wives and girlfriends of men who molest children--into the clear focus necessary to understand the dynamics of these disturbed families. Details of the study spotlight interview me作者: Ovulation 時(shí)間: 2025-3-22 14:17
Yutaka Hiraidinal and transverse wobbling modes in a single nucleus.EstaThis thesis presents significant new observations of nuclear wobbling, and thus expands our understanding of nuclear triaxiality and its prevalence in the nuclear chart. Triaxial nuclear shapes are a very rare phenomena and their experiment作者: Resection 時(shí)間: 2025-3-22 20:27 作者: 射手座 時(shí)間: 2025-3-22 21:45
ch als vernetztes Gro?system aber weiterhin im Wachstumsexze?. Dies ist kein auf die Medizin beschr?nktes Ph?nomen. Der Strom der Zeit ist rei?end geworden. So schreibt Sexl (1982, S. 239, 240): Krebsartig erscheint das Wachstum der Menschheit, ihres Energieverbrauches, ihres Materialkonsums, aber a作者: 協(xié)迫 時(shí)間: 2025-3-23 03:37 作者: Obstruction 時(shí)間: 2025-3-23 06:14
Yutaka Hirai both forms of wobbling in a single nucleus. Another important result reported in this work is the very first observation of co-existing chiral and wobbling modes in the .135.Pr nucleus. This thesis details the978-3-031-17152-9978-3-031-17150-5Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: photophobia 時(shí)間: 2025-3-23 11:07 作者: Carbon-Monoxide 時(shí)間: 2025-3-23 17:16 作者: 警告 時(shí)間: 2025-3-23 19:37
,Enrichment of ,-Process Elements in?Isolated Dwarf Galaxies,n galaxies with higher star formation efficiencies. The star-to-star scatters of the ratios of .-process elements to iron mainly come from the inhomogeneous spatial metallicity distribution in galaxies. The results demonstrate that it will be possible to estimate the early star formation histories o作者: Catheter 時(shí)間: 2025-3-24 00:22
Enrichment of ,-Process Elements in a Cosmological Context, early stages of galaxy formation. This result suggests that .-process rich stars seen in the Milky Way halo come from small size halos with the mass comparable to the Local Group ultra-faint dwarf galaxies.作者: athlete’s-foot 時(shí)間: 2025-3-24 03:03
2190-5053 ory of the early galaxies, and presents theoretical findings that open new avenues to understanding the formation and evolution of galaxies based on the abundance of heavy elements in metal-poor stars..978-981-13-7884-3Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: Iniquitous 時(shí)間: 2025-3-24 08:07 作者: 衍生 時(shí)間: 2025-3-24 12:04 作者: 收養(yǎng) 時(shí)間: 2025-3-24 18:02 作者: 褪色 時(shí)間: 2025-3-24 20:45 作者: 舊石器時(shí)代 時(shí)間: 2025-3-25 01:31 作者: Recessive 時(shí)間: 2025-3-25 06:58 作者: 隼鷹 時(shí)間: 2025-3-25 11:04
Understanding the Enrichment of Heavy Elements by the Chemodynamical Evolution Models of Dwarf Galax作者: 我不死扛 時(shí)間: 2025-3-25 13:31
Introduction,es. At the time of the big bang, the Universe consists of hydrogen, helium, and lithium. Explosive events such as supernovae and neutron star mergers distribute heavy elements to the interstellar medium. Dense gases containing these elements form stars. Abundances of heavy elements in stars, therefo作者: 演繹 時(shí)間: 2025-3-25 18:38 作者: 配置 時(shí)間: 2025-3-25 22:28 作者: debase 時(shí)間: 2025-3-26 00:27 作者: Resistance 時(shí)間: 2025-3-26 04:51 作者: Flat-Feet 時(shí)間: 2025-3-26 11:47 作者: 觀察 時(shí)間: 2025-3-26 13:38
Enrichment of ,-Process Elements in a Cosmological Context,th galaxy formation. In the hierarchical structure formation scenario, galaxies are thought to be formed by clustering of smaller systems. Star-to-star scatters of the ratios of .-process elements in the Milky Way halo should be reflected such process. However, the enrichment of .-process elements i作者: 變化 時(shí)間: 2025-3-26 18:27
Conclusions and Future Prospects,s. This book aims to understand (1) the contribution of neutron star mergers and supernovae (core-collapse supernovae, hypernovae, electron-capture supernovae, and type Ia supernovae) to the enrichment of heavy elements and (2) the relation between the chemodynamical evolution of galaxies and the ab作者: detach 時(shí)間: 2025-3-26 21:12 作者: scotoma 時(shí)間: 2025-3-27 01:49 作者: 連詞 時(shí)間: 2025-3-27 07:02 作者: SEED 時(shí)間: 2025-3-27 10:31 作者: 冷峻 時(shí)間: 2025-3-27 15:59 作者: deriver 時(shí)間: 2025-3-27 21:43 作者: 拾落穗 時(shí)間: 2025-3-27 22:30 作者: impale 時(shí)間: 2025-3-28 04:43 作者: Fermentation 時(shí)間: 2025-3-28 07:53
https://doi.org/10.1007/978-981-13-7884-3Galactic Chemical Evolution; Numerical Simulations of Galaxy Formation; Galactic Chemical Evolution; Fo作者: 清洗 時(shí)間: 2025-3-28 10:59
Yutaka HiraiNominated as an outstanding Ph.D thesis by the Department of Astronomy at the University of Tokyo.Includes a wealth of color figures to help readers understand ancient times in the Universe based on p作者: CODA 時(shí)間: 2025-3-28 15:21 作者: coltish 時(shí)間: 2025-3-28 20:51
Understanding the Enrichment of Heavy Elements by the Chemodynamical Evolution Models of Dwarf Galax978-981-13-7884-3Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: 下垂 時(shí)間: 2025-3-28 22:54
