Supernovae in Low-Redshift Galaxy Clusters: the Type-Ia Supernova Rate

Details Supernovae in Low-Redshift Galaxy Clusters: the Type-Ia Supernova Rate Supernovae in Low-Redshift Galaxy Clusters: the Type-Ia Supernova Rate

2006-10-08

arxiv.org/abs/astro-ph/0610228v2

Astrophys.J.660:1165-1175,2007

Astronomy and Astrophysics

Astrophysics

Revised version following referee's comments; Accepted by ApJ

Scientific paper

10.1086/513266

Supernova (SN) rates are a potentially powerful diagnostic of star formation history (SFH), metal enrichment, and SN physics, particularly in galaxy clusters with their deep, metal-retaining potentials, and simple SFH. However, a low-redshift cluster SN rate has never been published. We derive the SN rate in galaxy clusters at 0.06

Affiliated with

Also associated with

No associations

Rating

Supernovae in Low-Redshift Galaxy Clusters: the Type-Ia Supernova Rate 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 Supernovae in Low-Redshift Galaxy Clusters: the Type-Ia Supernova Rate, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Supernovae in Low-Redshift Galaxy Clusters: the Type-Ia Supernova Rate will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-517978