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Simulating the UV escape fractions from molecular...
Journal article

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 parameter which is vital to understanding the ionization of the ISM and the intergalactic medium. We characterize the escape fraction, fesc,GMC, from a suite of individual GMC simulations with masses in the range 104–6 M⊙ using the adaptive-mesh refinement code flash. We find significantly …

Authors

Howard CS; Pudritz RE; Harris WE; Klessen RS

Journal

Monthly Notices of the Royal Astronomical Society, Vol. 475, No. 3, pp. 3121–3134

Publisher

Oxford University Press (OUP)

Publication Date

April 11, 2018

DOI

10.1093/mnras/stx3276

ISSN

0035-8711