Neutron Stars, Pulsar Wind Nebulae, and their Supernovae

Details Neutron Stars, Pulsar Wind Nebulae, and their Supernovae Neutron Stars, Pulsar Wind Nebulae, and their Supernovae

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cfa..colle..11c&link_type=abstract

CfA Colloquium Lecture Series Talk

Mathematics

Scientific paper

Massive star supernovae can be divided into several categories depending on the amount of mass loss from the progenitor star and the star's radius. Various aspects of the immediate aftermath of the supernova are expected to develop in different ways depending on the supernova category; these aspects include mixing in the supernova, fallback on the central compact object, expansion of any pulsar wind nebula, interaction with circumstellar matter, and photoionization by shock breakout radiation. The observed properties of nearby young supernova remnants can be compared to the expectations for the different categories of supernovae.

Affiliated with

Also associated with

No associations

Rating

Neutron Stars, Pulsar Wind Nebulae, and their 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 Neutron Stars, Pulsar Wind Nebulae, and their Supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutron Stars, Pulsar Wind Nebulae, and their Supernovae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1387655