Supernova Remnants and their Progenitors

Details Supernova Remnants and their Progenitors Supernova Remnants and their Progenitors

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...9e..11d&link_type=abstract

Supernovae: One Millennium After SN1006, 26th meeting of the IAU, Joint Discussion 9, 17-18 August 2006, Prague, Czech Republic,

Computer Science

Scientific paper

Supernova remnants (SNRs) have a variety of different properties and come from progenitors with a range of masses and companions. I shall describe some of the morphologies and spectral properties over all wavelength bands plus environments of selected prototypical SNRs and discuss how we can attempt to relate them to their progenitors. Most young remnants, with a notable exception of Kepler 1604, can be successfully classified but after they have swept up about 8 times their ejected mass and entered the point-blast phase of their evolution, their parentage is more difficult to determine. Statistical arguments or the location of some form of neutron star within the remnant are the best indicators for the oldest remnants.

Affiliated with

Also associated with

No associations

Rating

Supernova Remnants and their Progenitors 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 Supernova Remnants and their Progenitors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Supernova Remnants and their Progenitors will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1784478