Dust Formation and Evolution in the Early Universe

Details Dust Formation and Evolution in the Early Universe Dust Formation and Evolution in the Early Universe

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005omeg.conf..509n&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2003. Held 17-19 November 2003 in RIKEN, Wako, Saitama, Japan. Edited by M Terasawa,

Astronomy and Astrophysics

Astronomy

Scientific paper

We have investigated the formation of dust grains in the ejecta of Population III supernova; core collapse supernovae with the progenitor mass Mpr ranging from 13 to 30 M&sun; and pair-instability supernovae with Mpr = 170 and 200 M&sun;. In this paper, we report the amount of dust grains formed in the ejecta of Population III supernovae, and discuss the time evolution of dust-to-gas mass ratio and metallicity in the primordial universe.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1466954