Observational selection, host galaxy dust, and Type Ia supernovae

Details Observational selection, host galaxy dust, and Type Ia supernovae Observational selection, host galaxy dust, and Type Ia supernovae

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004newar..48..567c&link_type=abstract

New Astronomy Reviews, Volume 48, Issue 7-8, p. 567-573.

Astronomy and Astrophysics

Astronomy

14

Supernovae, Dust, Host Galaxies, Observational Selection

Scientific paper

We develop models for extinction of Type Ia supernova light due to dust in spiral host galaxies. The models are based on well-known facts and concepts concerning galaxy morphology, star distributions, and dust. We find that observational selection causes extinctions of observable Ia supernovae to be very insensitive to large variations in host galaxy dust, especially at high redshift.

Affiliated with

Also associated with

No associations

Rating

Observational selection, host galaxy dust, and Type Ia 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 Observational selection, host galaxy dust, and Type Ia supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observational selection, host galaxy dust, and Type Ia supernovae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1552254