XMM-Newton Proposal 03018809

Details XMM-Newton Proposal 03018809 XMM-Newton Proposal 03018809

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...62k&link_type=abstract

XMM-Newton Proposal ID #03018809

Computer Science

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, G6.1+1.2, G18.9-1.1, G24.7+0.6, G27.8+0.6, G30.7+1.0, G73.9+0.9, G318.9+0.4, G341.2+0.9, G28.8+1.5, Xmm-Newton Proposal 03018809

Scientific paper

Supernova Remnants of center-filled and composite types often host young, energetic pulsars emitting strong relativistic winds. XMM-Newton and Chandra observations of such SNRs have already resulted in a number of pulsar and pulsar-wind nebula (PWN) discoveries. We propose to observe the remaining plerionic remnants located within a distance of 7 kpc. The SNRs were selected based on their radio morphologies and serendipitous ROSAT or ASCA data. This survey will substantially expand the sample of PNWe and pulsars observed in X-rays and help to establish the properties of the overall population.

Affiliated with

Also associated with

No associations

Rating

XMM-Newton Proposal 03018809 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 XMM-Newton Proposal 03018809, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and XMM-Newton Proposal 03018809 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1474032