Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-11-04
Astronomy and Astrophysics
Astrophysics
7 pages, 3 figures; to be published in 'Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology', 2006, ASP Con
Scientific paper
How much dust can be produced in the early Universe? Does dust production depend on the average heavy-metal content of the hosting galaxy? Considering supernova explosions, massive stars (Wolf-Rayet, LBV and RSG), and relatively massive AGB stars among possible dust-generating objects in the early Universe, we find that SN remnants can be regarded as the main source of the primordial dust. However, this conclusion is based on highly uncertain (and probably over-estimated) dust production rates. Despite all the uncertainties, interstellar extinction must be taken into account while observing high-redshift objects.
No associations
LandOfFree
Dust Production in the High-Redshift Universe 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 Production in the High-Redshift Universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dust Production in the High-Redshift Universe will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-419043