The Bizarre Young Supernova Remnant G350.1-0.3

Details The Bizarre Young Supernova Remnant G350.1-0.3 The Bizarre Young Supernova Remnant G350.1-0.3

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...79g&link_type=abstract

XMM-Newton Proposal ID #04020401

Physics

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, G350.1-0.3, Xmm-Newton Proposal 04020401

Scientific paper

Supernova remnants (SNRs) with unusual morphologies indicate complicated interactions with their surroundings, demonstrating the wide variety of conditions into which supernovae explode. G350.1-0.3 is a long-overlooked radio and X-ray source with a bizarre morphology, which we argue is a very young and luminous SNR expanding into dense ambient gas. We here propose imaging and spectroscopic observations of G350.1-0.3 with XMM, through which we can probe the physical conditions in this SNR and begin to understand its interaction with its surroundings.

Affiliated with

Also associated with

No associations

Rating

The Bizarre Young Supernova Remnant G350.1-0.3 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 Bizarre Young Supernova Remnant G350.1-0.3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Bizarre Young Supernova Remnant G350.1-0.3 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1659888