Dust Formation in Damped LYalpha Systems

Details Dust Formation in Damped LYalpha Systems Dust Formation in Damped LYalpha Systems

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26at...21..265k&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 21, Issue 4, p.265-269

Astronomy and Astrophysics

Astrophysics

Scientific paper

A one-zone spectrophotometric and chemical evolution scenario of spiral galaxies incorporating dust formation is briefly described, and a self-consistent closed box chemical model of the gaseous disks (corrected on dust depletion) is presented. Comparison of the calculated abundances with the observed in damped Lyf systems shows first, that at least a fraction of DLA absorptions can be attributed to spiral galaxies, and that the dust is a nessasary physical ingredient of galaxy evolution model strongly affecting the observed abundance pattern and photometric properties.

Affiliated with

Also associated with

No associations

Rating

Dust Formation in Damped LYalpha Systems 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 Formation in Damped LYalpha Systems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dust Formation in Damped LYalpha Systems will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1533601