Chemo-dynamical evolution of galaxies

Details Chemo-dynamical evolution of galaxies Chemo-dynamical evolution of galaxies

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170..231h&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astrophysics

12

Astronomical Models, Galactic Evolution, Interstellar Matter, Star Formation, Stellar Composition, Dwarf Galaxies, Dynamic Models, Metallicity, Stellar Mass Ejection, Stellar Winds

Scientific paper

The evolution of galaxies is investigated, taking into account a detailed description of the stars and a multi-component interstellar medium as well as their interactions. Since cooling and heating processes determine the dynamical evolution of galaxies but depend on the metal content, dynamical and chemical evolution are intimately coupled. First, the models show that different initial conditions can account for several observed properties and the different types of galaxies and, secondly, that most galaxies experience repeated star-formation bursts on time-scales which also depend on the initial conditions.

Affiliated with

Also associated with

No associations

Rating

Chemo-dynamical evolution of 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 Chemo-dynamical evolution of galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chemo-dynamical evolution of galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1124902