书目名称 | Lyman-alpha as an Astrophysical and Cosmological Tool | 副标题 | Saas-Fee Advanced Co | 编辑 | Mark Dijkstra,J. Xavier Prochaska,Matthew Hayes,An | 视频video | | 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 | 丛书名称 | Saas-Fee Advanced Course | 图书封面 |  | 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 | 关键词 | resonance line transfer; high-redshift galaxies; Lyman-alpha forest; galaxy formation; galaxy evolution; | 版次 | 1 | doi | https://doi.org/10.1007/978-3-662-59623-4 | isbn_softcover | 978-3-662-59625-8 | isbn_ebook | 978-3-662-59623-4Series ISSN 1861-7980 Series E-ISSN 1861-8227 | issn_series | 1861-7980 | copyright | Springer-Verlag GmbH Germany, part of Springer Nature 2019 |
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