Dust SED Model of Very Young Galaxies with AGB-Star Dust

Details Dust SED Model of Very Young Galaxies with AGB-Star Dust Dust SED Model of Very Young Galaxies with AGB-Star Dust

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aspc..445..551t&link_type=abstract

Why Galaxies Care about AGB Stars II: Shining Examples and Common Inhabitants. Proceedings of a conference held at University Ca

Astronomy and Astrophysics

Astronomy

Scientific paper

Recently, it has been found that the contribution of dust from AGB stars is significant even if the galaxy is very young (age < 1 Gyr). We show a dust SED model including the emission from dust from AGB stars based on our new dust evolution scenario. The AGB-star dust contribution increases the infrared luminosity of galaxies after the age of several × 108 yr.

Affiliated with

Also associated with

No associations

Rating

Dust SED Model of Very Young Galaxies with AGB-Star Dust 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 SED Model of Very Young Galaxies with AGB-Star Dust, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dust SED Model of Very Young Galaxies with AGB-Star Dust will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-829513