The Radio Counterpart of the X-ray Pulsar Wind Nebula in the SNR G0.9+0.1

Details The Radio Counterpart of the X-ray Pulsar Wind Nebula in the SNR G0.9+0.1 The Radio Counterpart of the X-ray Pulsar Wind Nebula in the SNR G0.9+0.1

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006esasp.604..365d&link_type=abstract

Proceedings of the The X-ray Universe 2005 (ESA SP-604). 26-30 September 2005, El Escorial, Madrid, Spain. Editor: A. Wilson, p.

Physics

Scientific paper

We report on new radio observations of the central nebula in the SNR G0.9+0.1 at 4.8 GHz and 8.6 GHz. These data unveil a highly clumpy structure of the radio nebula. Most of the radio features are uncorrelated with the X-ray emission. Not any point-like radio source is detected at the position of CXOU J174722.8-280915, the proposed neutron star. On the contrary, the X-ray source seems to lie within a small minimum in the radio emission.

Affiliated with

Also associated with

No associations

Rating

The Radio Counterpart of the X-ray Pulsar Wind Nebula in the SNR G0.9+0.1 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 Radio Counterpart of the X-ray Pulsar Wind Nebula in the SNR G0.9+0.1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Radio Counterpart of the X-ray Pulsar Wind Nebula in the SNR G0.9+0.1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1207166