Cosmological Models and the Brightness Profile of Distant Galaxies

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

4 pages, no figures. Contributed paper presented at IAU 2009, Rio de Janeiro, Brazil. Typos corrected

Scientific paper

The aim of this project is to determine the consistency of an assumed cosmological model by means of a detailed analysis of the brightness profiles of distant galaxies.Starting from the theory developed by Ellis and Perry (1979) connecting the angular diameter distance obtained from a relativistic cosmological model and the detailed photometry of galaxies, we assume the presently most accepted cosmological model with non-zero cosmological constant and attempt to predict the brightness profiles of galaxies of a given redshift. Then this theoretical profile can be compared to observational data already available for distant, that is, high redshift, galaxies. By comparing these two curves we may reach conclusions about the observational feasibility of the underlying cosmological model.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Cosmological Models and the Brightness Profile of Distant 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 Cosmological Models and the Brightness Profile of Distant Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmological Models and the Brightness Profile of Distant Galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-499270

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.