標(biāo)題: Titlebook: Lyman-alpha as an Astrophysical and Cosmological Tool; Saas-Fee Advanced Co Mark Dijkstra,J. Xavier Prochaska,Matthew Hayes,An Book 2019 Sp [打印本頁] 作者: 徽章 時(shí)間: 2025-3-21 16:20
書目名稱Lyman-alpha as an Astrophysical and Cosmological Tool影響因子(影響力)
書目名稱Lyman-alpha as an Astrophysical and Cosmological Tool影響因子(影響力)學(xué)科排名
書目名稱Lyman-alpha as an Astrophysical and Cosmological Tool網(wǎng)絡(luò)公開度
書目名稱Lyman-alpha as an Astrophysical and Cosmological Tool網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Lyman-alpha as an Astrophysical and Cosmological Tool被引頻次
書目名稱Lyman-alpha as an Astrophysical and Cosmological Tool被引頻次學(xué)科排名
書目名稱Lyman-alpha as an Astrophysical and Cosmological Tool年度引用
書目名稱Lyman-alpha as an Astrophysical and Cosmological Tool年度引用學(xué)科排名
書目名稱Lyman-alpha as an Astrophysical and Cosmological Tool讀者反饋
書目名稱Lyman-alpha as an Astrophysical and Cosmological Tool讀者反饋學(xué)科排名
作者: BOLT 時(shí)間: 2025-3-21 21:29
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作者: 蕨類 時(shí)間: 2025-3-22 03:11 作者: CHOKE 時(shí)間: 2025-3-22 05:17
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作者: Ejaculate 時(shí)間: 2025-3-22 12:42
Lyman-alpha as an Astrophysical and Cosmological ToolSaas-Fee Advanced Co作者: Permanent 時(shí)間: 2025-3-22 14:06
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作者: ordain 時(shí)間: 2025-3-22 17:44
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.作者: engagement 時(shí)間: 2025-3-22 22:58
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作者: 沉著 時(shí)間: 2025-3-23 02:57 作者: 觀察 時(shí)間: 2025-3-23 05:43
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 作者: 審問,審訊 時(shí)間: 2025-3-23 13:21 作者: GUILT 時(shí)間: 2025-3-23 17:44 作者: Melanocytes 時(shí)間: 2025-3-23 18:40 作者: 憲法沒有 時(shí)間: 2025-3-24 00:17 作者: Trabeculoplasty 時(shí)間: 2025-3-24 05:18
978-3-662-59625-8Springer-Verlag GmbH Germany, part of Springer Nature 2019作者: defray 時(shí)間: 2025-3-24 08:50
Lyman-alpha as an Astrophysical and Cosmological Tool978-3-662-59623-4Series ISSN 1861-7980 Series E-ISSN 1861-8227 作者: Neutropenia 時(shí)間: 2025-3-24 12:01 作者: glacial 時(shí)間: 2025-3-24 17:44 作者: flourish 時(shí)間: 2025-3-24 20:26 作者: 披肩 時(shí)間: 2025-3-24 23:53
Physics of Ly, Radiative Transfer,or anyone with an undergraduate degree in astronomy/physics. Throughout these notes, I denote symbols that represent vectors in .. Throughout I will use CGS units, as is common in the literature. Table?. provides an overview of (some of the) symbols that appear throughout these notes.作者: 思鄉(xiāng)病 時(shí)間: 2025-3-25 05:44 作者: 硬化 時(shí)間: 2025-3-25 11:03
-convection-diffusion problems exhibiting layer behaviour. More precisely, it is devoted to the construction and analysis of layer-adapted meshes underlying these numerical methods. Numerical methods for singularly perturbed differential equations have been studied since the early 1970s and the rese作者: 創(chuàng)作 時(shí)間: 2025-3-25 14:00
Mark Dijkstra-convection-diffusion problems exhibiting layer behaviour. More precisely, it is devoted to the construction and analysis of layer-adapted meshes underlying these numerical methods. Numerical methods for singularly perturbed differential equations have been studied since the early 1970s and the rese作者: Friction 時(shí)間: 2025-3-25 16:15 作者: fringe 時(shí)間: 2025-3-25 21:32
Masami Ouchiayer behaviour. More precisely, it is devoted to the construction and analysis of layer-adapted meshes underlying these numerical methods. Numerical methods for singularly perturbed differential equations have been studied since the early 1970s and the research frontier has been constantly - panding作者: 恫嚇 時(shí)間: 2025-3-26 04:08 作者: Ptsd429 時(shí)間: 2025-3-26 05:52
Mark Dijkstraayer behaviour. More precisely, it is devoted to the construction and analysis of layer-adapted meshes underlying these numerical methods. Numerical methods for singularly perturbed differential equations have been studied since the early 1970s and the research frontier has been constantly - panding作者: 鎮(zhèn)痛劑 時(shí)間: 2025-3-26 10:55 作者: 縱火 時(shí)間: 2025-3-26 15:55
Physics of Ly, Radiative Transfer, statistics, statistical physics/thermodynamics, computational astrophysics, and has applications in a wide range of astrophysical contexts including galaxies, the interstellar medium, the circum-galactic medium, the intergalactic medium, reionization, 21-cm cosmology and astrophysics. In these lect作者: 產(chǎn)生 時(shí)間: 2025-3-26 16:55
H, Absorption in the Intergalactic Medium,udies. The chapter begins with a historical perspective and then offers a pedagogical description of the quantum mechanics underlying the Lyman series and Lyman continuum opacity of the H. atom. We describe the manifestation of these opacities in absorption spectroscopy and the challenges related to作者: 努力趕上 時(shí)間: 2025-3-27 00:44
Observations of Ly, Emitters at High Redshift, of LAEs in the late 1990s, significant progresses in LAE studies have been made over the past two decades by deep multi-wavelength observations. More than ten thousands of LAEs have been identified photometrically, and more than one thousand spectroscopically, in optical and near-infrared data, and作者: STING 時(shí)間: 2025-3-27 01:56
Lyman Alpha Emission and Absorption in Local Galaxies,n motivations, astrophysical prerequisites, and definitions. Section 2 describes the various instruments that have contributed to the field or are currently capable of observing Ly. at ., and their basic characteristics. Section 3 is concerned with the first generation of Ly. observations of quasars作者: 憂傷 時(shí)間: 2025-3-27 07:39
9樓作者: filicide 時(shí)間: 2025-3-27 11:10
10樓作者: 撤退 時(shí)間: 2025-3-27 15:12
10樓作者: CONE 時(shí)間: 2025-3-27 20:46
10樓作者: Pepsin 時(shí)間: 2025-3-28 01:50
10樓
