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Titlebook: Lyman-alpha as an Astrophysical and Cosmological Tool; Saas-Fee Advanced Co Mark Dijkstra,J. Xavier Prochaska,Matthew Hayes,An Book 2019 Sp

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發(fā)表于 2025-3-21 16:20:32 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱(chēng)Lyman-alpha as an Astrophysical and Cosmological Tool
副標(biāo)題Saas-Fee Advanced Co
編輯Mark Dijkstra,J. Xavier Prochaska,Matthew Hayes,An
視頻videohttp://file.papertrans.cn/590/589183/589183.mp4
概述Fills a gap of graduate lecture books dedicated to this topic.Gathers state-of-the art theory and observations.Discusses main science case of several forthcoming facilities.Presents elaborated lecture
叢書(shū)名稱(chēng)Saas-Fee Advanced Course
圖書(shū)封面Titlebook: Lyman-alpha as an Astrophysical and Cosmological Tool; Saas-Fee Advanced Co Mark Dijkstra,J. Xavier Prochaska,Matthew Hayes,An Book 2019 Sp
描述.The hydrogen Lyman-alpha line is of utmost importance to many fields of astrophysics. This UV line being conveniently redshifted with distance to the visible and even near infrared wavelength ranges, it is observable from the ground, and provides the main observational window on the formation and evolution of high redshift galaxies. Absorbing systems that would otherwise go unnoticed are revealed through the Lyman-alpha forest, Lyman-limit, and damped Lyman-alpha systems, tracing the distribution of baryonic matter on large scales, and its chemical enrichment..We are living an exciting epoch with the advent of new instruments and facilities, on board of satellites and on the ground. Wide field and very sensitive integral field spectrographs are becoming available on the ground, such as MUSE at the ESO VLT. The giant E-ELT and TMT telescopes will foster a quantum leap in sensitivity and both spatial and spectroscopic resolution, to the point of being able, perhaps, to measure directly the acceleration of the Hubble flow. In space, the JWST will open new possibilities to study the Lyman-alpha emission of primordial galaxies in the near infrared. As long as the Hubble Space Telescope
出版日期Book 2019
關(guān)鍵詞resonance line transfer; high-redshift galaxies; Lyman-alpha forest; galaxy formation; galaxy evolution;
版次1
doihttps://doi.org/10.1007/978-3-662-59623-4
isbn_softcover978-3-662-59625-8
isbn_ebook978-3-662-59623-4Series ISSN 1861-7980 Series E-ISSN 1861-8227
issn_series 1861-7980
copyrightSpringer-Verlag GmbH Germany, part of Springer Nature 2019
The information of publication is updating

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發(fā)表于 2025-3-21 21:29:11 | 只看該作者
Matthew Hayess of special meshes was made by N.S. Bakhvalov [18] in 1969. His paper spawned a lively discussion in the literature with a number of further meshes - ing proposed and applied to various singular perturbation problems. However, in the mid 1980s, this development stalled, but was enlivened again by G
板凳
發(fā)表于 2025-3-22 03:11:48 | 只看該作者
地板
發(fā)表于 2025-3-22 05:17:36 | 只看該作者
s of special meshes was made by N.S. Bakhvalov [18] in 1969. His paper spawned a lively discussion in the literature with a number of further meshes - ing proposed and applied to various singular perturbation problems. However, in the mid 1980s, this development stalled, but was enlivened again by G
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發(fā)表于 2025-3-22 12:42:50 | 只看該作者
Lyman-alpha as an Astrophysical and Cosmological ToolSaas-Fee Advanced Co
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發(fā)表于 2025-3-22 14:06:45 | 只看該作者
Observations of Ly, Emitters at High Redshift,. Typical LAEs represent low-mass high-. galaxies, high-. analogs of dwarf galaxies, some of which are thought to be candidates of population III galaxies. These observational studies have also pinpointed rare bright Ly. sources extended over .–100?kpc, dubbed Ly. blobs, whose physical origins are u
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發(fā)表于 2025-3-22 17:44:37 | 只看該作者
Lyman Alpha Emission and Absorption in Local Galaxies,ions and the existence of large-scale Ly. halos. Section 7 endeavors to present a unifying scenario for Ly. emission from galaxies, synthesizes the results, and discusses what we would like to know from the next generation of observations.
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發(fā)表于 2025-3-22 22:58:49 | 只看該作者
Book 2019both spatial and spectroscopic resolution, to the point of being able, perhaps, to measure directly the acceleration of the Hubble flow. In space, the JWST will open new possibilities to study the Lyman-alpha emission of primordial galaxies in the near infrared. As long as the Hubble Space Telescope
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發(fā)表于 2025-3-23 02:57:49 | 只看該作者
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發(fā)表于 2025-3-23 05:43:28 | 只看該作者
Mark Dijkstraiterature with a number of further meshes - ing proposed and applied to various singular perturbation problems. However, in the mid 1980s, this development stalled, but was enlivened again by G978-3-642-05133-3978-3-642-05134-0Series ISSN 0075-8434 Series E-ISSN 1617-9692
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