Classifications of the Host Galaxies of Supernovae, Set III

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Accepted for publishing in PASP

Scientific paper

10.1086/431435

A homogeneous sample comprising host galaxies of 604 recent supernovae, including 212 objects discovered primarily in 2003 and 2004, has been classified on the David Dunlap Observatory system. Most SN 1991bg-like SNe Ia occur in E and E/Sa galaxies, whereas the majority of SN 1991T-like SNe Ia occur in intermediate-type galaxies. This difference is significant at the 99.9% level. As expected, all types of SNe II are rare in early-type galaxies, whereas normal SNe Ia occur in all Hubble types. This difference is significant at the 99.99% level. A small number of SNe II in E galaxies might be due to galaxy classification errors, or to a small young-population component in these mainly old objects. No significant difference is found between the distributions over Hubble type of SNe Ibc and SNe II. This confirms that both of these types of objects have similar (massive) progenitors. The present data show that, in order to understand the dependence of supernova type on host-galaxy population, it is more important to obtain accurate morphological classifications than it is to increase the size of the data sample.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Classifications of the Host Galaxies of Supernovae, Set III 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 Classifications of the Host Galaxies of Supernovae, Set III, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Classifications of the Host Galaxies of Supernovae, Set III will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-402906

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.