Simulating the UV escape fractions from molecular cloud populations in star-forming dwarf and spiral galaxies

Abstract. The escape of ultraviolet photons from the densest regions of the interstellar medium (ISM) - giant molecular clouds (GMCs) - is a poorly constrained

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Bibliographic Details
Main Authors: Howard, Corey S. (Author) , Pudritz, Ralph E. (Author) , Klessen, Ralf S. (Author)
Format: Article (Journal)
Language:English
Published: 2018
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 475, Issue: 3, Pages: 3121-3134
ISSN:1365-2966
DOI:10.1093/mnras/stx3276
Online Access:Verlag, Volltext: https://doi.org/10.1093/mnras/stx3276
Verlag, Volltext: https://academic.oup.com/mnras/article/475/3/3121/4768292
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Author Notes:Corey S. Howard, Ralph E. Pudritz, William E. Harris, Ralf S. Klessen
Description
Summary:Abstract. The escape of ultraviolet photons from the densest regions of the interstellar medium (ISM) - giant molecular clouds (GMCs) - is a poorly constrained
Item Description: Published: 20 December 2017
Gesehen am 09.10.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stx3276