Dust Attenuation in Bulge+Disk Systems

Details Dust Attenuation in Bulge+Disk Systems Dust Attenuation in Bulge+Disk Systems

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..17..200p&link_type=abstract

Galaxy Evolution: Theory & Observations (Eds. Vladimir Avila-Reese, Claudio Firmani, Carlos S. Frenk & Christine Allen) Revista

Astronomy and Astrophysics

Astronomy

2

Dust, Extinction, Galaxies: Spiral, Methods: Numerical, Radiative Transfer

Scientific paper

We present new Monte-Carlo radiative transfer calculations aimed at
quantifying the dust effects (absorption and scattering) on the total
UV/optical/near-IR continuum emission from the stellar populations of an
Sbc galaxy like the Milky Way (MW) and of its individual bulge and disk
components, as a function of dust content and galaxy inclination.

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