Supernova Remnants in the Halo

Details Supernova Remnants in the Halo Supernova Remnants in the Halo

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...188.7405s&link_type=abstract

American Astronomical Society, 188th AAS Meeting, #74.05; Bulletin of the American Astronomical Society, Vol. 28, p.948

Astronomy and Astrophysics

Astronomy

Scientific paper

Observations tell us that the halo contains high stage ions such as C(+3) , N(+4) , and O(+5) and even higher ions responsible for x-ray emission. Therefore, a significant, but poorly determined, fraction of the halo's volume must be hot. Various theoretical scenarios predict hot gas in the halo. In this work, we are interested in more accurately determining the contributions made by isolated, halo supernova remnants. A one-dimensional, Lagrangian, hydrodynamic code is used to simulated the long term evolution of the halo supernova remnants. The resulting high ion and x-ray contributions are presented.

Affiliated with

Also associated with

No associations

Rating

Supernova Remnants in the Halo 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 Supernova Remnants in the Halo, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Supernova Remnants in the Halo will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1355550