A Chandra Study of the Interaction between the Plasma Nebula RCW89 and the pulsar jet of PSR B1509-58

Details A Chandra Study of the Interaction between the Plasma Nebula RCW89 and the pulsar jet of PSR B1509-58 A Chandra Study of the Interaction between the Plasma Nebula RCW89 and the pulsar jet of PSR B1509-58

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cxo..prop.1713y&link_type=abstract

Chandra Proposal ID #06500799

Computer Science

Chandra Proposal Id #06500799

Scientific paper

RCW89 is part of the supernova remnant G320.4-01.2 with the young pulsar PSR B1509-58 accompanied by the pulsar wind nebula and jet features. Since RCW89 is located at the terminus of the jet, it has been suggested that the plasma nebulae are powered by the precessing pulsar-jet. In order to determine the dynamics of pulsar jets and the secular change of plasma nebula, we will compare this observation with the past Chandra data of this region on Aug 14, 2000.

Affiliated with

Also associated with

No associations

Rating

A Chandra Study of the Interaction between the Plasma Nebula RCW89 and the pulsar jet of PSR B1509-58 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 A Chandra Study of the Interaction between the Plasma Nebula RCW89 and the pulsar jet of PSR B1509-58, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Chandra Study of the Interaction between the Plasma Nebula RCW89 and the pulsar jet of PSR B1509-58 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1063518