STRESS Counting Supernovae

Details STRESS Counting Supernovae STRESS Counting Supernovae

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008msngr.134...25b&link_type=abstract

The Messenger, vol. 134, p. 25-29

Physics

Scientific paper

The rate of occurrence of supernovae (SNe) is linked to some of the basic ingredients of galaxy evolution, such as the star formation rate, the chemical enrichment and feedback processes. SN rates at intermediate redshift and their dependence on specific galaxy properties have been investigated in the Southern inTermediate Redshift ESO Supernova Search (STRESS). The rate of core collapse SNe (CC SNe) at a redshift of around 0.25 is found to be a factor two higher than the local value, whereas the SNe Ia rate remains almost constant. SN rates in red and blue galaxies were also measured and it was found that the SNe Ia rate seems to be constant in galaxies of different colour, whereas the CC SN rate seems to peak in blue galaxies, as in the local Universe.

Affiliated with

Also associated with

No associations

Rating

STRESS Counting Supernovae 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 STRESS Counting Supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and STRESS Counting Supernovae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-794193