Resonance line transfer in clumpy media
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/344/2/553/3909827/344-2-553.pdf
Reference27 articles.
1. A New High-Redshift L[CLC]y[/CLC]α Emitter: Possible Superwind Galaxy at [ITAL][CLC]z[/CLC][/ITAL] = 5.69
2. Jet‐induced Emission‐Line Nebulosity and Star Formation in the High‐Redshift Radio Galaxy 4C 41.17
3. Attenuation of Lyman-alpha emission by dust in damped Lyman-alpha systems
4. A Galactic Wind at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z=5.190$ \end{document}
5. Optical properties of interstellar graphite and silicate grains
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1. Deciphering the Lyman-α emission line: towards the understanding of galactic properties extracted from Lyα spectra via radiative transfer modelling;Monthly Notices of the Royal Astronomical Society;2022-04-30
2. Lyα Radiative Transfer: Modeling Spectrum and Surface Brightness Profiles of Lyα-emitting Galaxies at Z = 3–6;The Astrophysical Journal;2020-09-01
3. Lymanαline and continuum radiative transfer in a clumpy interstellar medium;Astronomy & Astrophysics;2014-02
4. ON THE (NON-)ENHANCEMENT OF THE Lyα EQUIVALENT WIDTH BY A MULTIPHASE INTERSTELLAR MEDIUM;The Astrophysical Journal;2013-03-15
5. B2 0902+34: A COLLAPSING PROTOGIANT ELLIPTICAL GALAXY ATz= 3.4;The Astrophysical Journal;2009-03-16
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