Dust evolution in gas-rich galaxies

Details Dust evolution in gas-rich galaxies Dust evolution in gas-rich galaxies

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..761..145k&link_type=abstract

THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop. AIP Conference Pr

Physics

1

Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, Spiral Galaxies

Scientific paper

We present a numerical model which simultaneously calculates the spectrophotometric evolution of gas-rich galaxies together with the chemical and dust evolution of their interstellar medium. For spiral galaxies the corresponding influence of dust evolution on SEDs, colors, and heavy element abundances in the gaseous phase is studied in detail. Confronting model results for spiral galaxies with the chemical abundances observed in Damped Ly-alpha Systems, we conclude that spiral galaxies may be considered as DLAs absorbers.

Affiliated with

Also associated with

No associations

Rating

Dust evolution in gas-rich galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Dust evolution in gas-rich galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dust evolution in gas-rich galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1453571