No CrossRef data available.
Article contents
Effects of Dust Extinction in Galactic Discs
Published online by Cambridge University Press: 25 May 2016
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
We have solved the radiative transfer equation taking into account both absorption and scattering into the line of sight to the observer to model the disc of spiral galaxies.
A dust model has been adopted, suitable for the diffuse interstellar medium of our Galaxy, to obtain, in aU the considered spectral range (1000 ÷ 10000 Å), consistent quantities to describe both the absorption and the scattering properties of the dust.
- Type
- Poster Papers
- Information
- Copyright
- Copyright © Kluwer 1996