Shock Physics Revealed by SN1006 Ejecta Knot

Details Shock Physics Revealed by SN1006 Ejecta Knot Shock Physics Revealed by SN1006 Ejecta Knot

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0503k&link_type=abstract

American Astronomical Society, HEAD meeting #9, #5.03; Bulletin of the American Astronomical Society, Vol. 38, p.348

Astronomy and Astrophysics

Astronomy

Scientific paper

The interaction with the ISM surrounding a Supernova remnant has been well modeled however recent x-ray observations of SN1006 reveal a protrusion of ejecta contrary to current remnant evolution and blast wave models. FUSE data reveal O VI intensities and line profiles that indicate the ejecta is moving faster than 3000 km/sec. Using this data with the Chandra and XMM observations of the same knot, we will describe the heating and temperature equilibration between the ion, electrons and protons at this shock front. This work was funded by FUSE grant.

Affiliated with

Also associated with

No associations

Rating

Shock Physics Revealed by SN1006 Ejecta Knot 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 Shock Physics Revealed by SN1006 Ejecta Knot, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Shock Physics Revealed by SN1006 Ejecta Knot will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-776760