Astronomy and Astrophysics – Astrophysics
Scientific paper
1993-06-23
Astrophys.J.417:54,1993
Astronomy and Astrophysics
Astrophysics
29 pages, incl 6 figures. Stone-age postscript replaced by LATeX. Latest version at http://www.sns.ias.edu/~max/gp.html (faste
Scientific paper
10.1086/173290
A model is presented in which supernova-driven winds from early galaxies reionize the intergalactic medium by z=5. This scenario can explain the observed absence of a Gunn-Peterson trough in the spectra of high-redshift quasars providing that the bulk of these early galaxies are quite small, no more massive than about 10^8 solar masses. It also predicts that most of the IGM was enriched to at least 10% of current metal content by z=5 and perhaps as early as z=15. The existence of such early mini-galaxies violates no spectral constraints and is consistent with a pure CDM model with b<2. Since the final radius of a typical ionized bubble is only around 100 kpc, the induced modification of the galaxy autocorrelation function is negligible, as is the induced angular smoothing of the CMBR. Some of the gas swept up by shells may be observable as pressure-supported Lyman-alpha forest clouds.
Evrard August
Silk Joseph
Tegmark Max
No associations
LandOfFree
Late reionization by supernova-driven winds 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 Late reionization by supernova-driven winds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Late reionization by supernova-driven winds will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-163042