Photometric evolution of N-body + SPH + star formation simulations of isolated disc galaxies

Details Photometric evolution of N-body + SPH + star formation simulations of isolated disc galaxies Photometric evolution of N-body + SPH + star formation simulations of isolated disc galaxies

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.284..921m&link_type=abstract

Astrophysics and Space Science, v. 284, Issue 2, p. 921-924 (2003).

Astronomy and Astrophysics

Astrophysics

1

N-Body Simulations, Disc Galaxies, Photometric Evolution

Scientific paper

We have calibrated self-consistent simulations of isolated disc galaxies including star, gas and star formation with the spectro-photometric evolutionary model GISSEL2000 (Bruzual and Charlot, 1993). With this approach we can compare morphologies studying mass and luminous distributions. We present an example about the evolution of bar ellipticity, which is simultaneously governed by dynamic and spectro-photometric evolution.

Affiliated with

Also associated with

No associations

Rating

Photometric evolution of N-body + SPH + star formation simulations of isolated disc 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 Photometric evolution of N-body + SPH + star formation simulations of isolated disc galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometric evolution of N-body + SPH + star formation simulations of isolated disc galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-919685