The far-infrared properties of parent galaxies of supernovae

Details The far-infrared properties of parent galaxies of supernovae The far-infrared properties of parent galaxies of supernovae

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...261..433p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 261, no. 2, p. 433-442.

Astronomy and Astrophysics

Astronomy

8

Far Infrared Radiation, Spiral Galaxies, Supernovae, Infrared Astronomy Satellite, Massive Stars, Star Distribution, Stellar Luminosity

Scientific paper

The far-infrared properties of the parent galaxies of supernovae are studied using the multivariate factor analysis of two samples of IRAS detected spiral galaxies: the parent galaxies of SNe and the RSA galaxies without recorded SN. The FIR parameters are found to be independent of the SNe with massive progenitors, the morphological type and the presence of the bar, as well as the blue luminosity of the galaxies. These results suggest that different ranges of mass dominate the optical and the FIR bands. The SN II is considered to be associated with the cooler component of the FIR radiation of galaxies and the masses of their projectors are restricted between 5 and 10 solar masses.

Affiliated with

Also associated with

No associations

Rating

The far-infrared properties of parent galaxies of 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 The far-infrared properties of parent galaxies of supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The far-infrared properties of parent galaxies of supernovae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1164067