Chemical Evolution in the Early Universe: Can Damp Lyα Systems Be Spiral Galaxies?

Details Chemical Evolution in the Early Universe: Can Damp Lyα Systems Be Spiral Galaxies? Chemical Evolution in the Early Universe: Can Damp Lyα Systems Be Spiral Galaxies?

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263...71d&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 71-74 (1998).

Astronomy and Astrophysics

Astrophysics

Scientific paper

The distribution of element abundances with redshift in Damped Lyα (DLA) systems can be adequately reproduced by the same models reproducing the halo and disk components of the Milky Way Galaxy at different galactocentric distances. In this sense, DLA systems are well represented by normal spiral galaxies in their early evolutionary stages.

Affiliated with

Also associated with

No associations

Rating

Chemical Evolution in the Early Universe: Can Damp Lyα Systems Be Spiral 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 Chemical Evolution in the Early Universe: Can Damp Lyα Systems Be Spiral Galaxies?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chemical Evolution in the Early Universe: Can Damp Lyα Systems Be Spiral Galaxies? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1330968