Supernova Remnants in X-Rays and Infrared: 0453.1-66.55 and DEM L204

Details Supernova Remnants in X-Rays and Infrared: 0453.1-66.55 and DEM L204 Supernova Remnants in X-Rays and Infrared: 0453.1-66.55 and DEM L204

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..144b&link_type=abstract

XMM-Newton Proposal ID #05037101

Physics

Supernovae, Supernova Remnants, Diffuse (Galactic) Emission And Isolated Neutron Stars, 0453.1-66.55, Xmm-Newton Proposal 05037101

Scientific paper

Recent observations of supernova remnants (SNR) with the Spitzer Space Telescope revealed that thermal dust emission dominates their infrared (IR) spectra. IR emission was detected mostly in X-ray bright SNRs, but it is also present in several older and fainter SNRs. We propose an X-ray study of two such IR remnants, 0453.1-66.55 and DEM L204. The origin of IR emission and the nature of these SNRs are not understood. X-ray imaging with the XMM-Newton EPIC camera will reveal location of the hot gas relative to optical and IR emission, allowing us to understand the origin of the IR emission. X-ray spectroscopy will provide as with temperatures and abundances of the hot gas. We will learn about dust content, energetics, and the evolutionary state of these unusual infrared SNRs.

Affiliated with

Also associated with

No associations

Rating

Supernova Remnants in X-Rays and Infrared: 0453.1-66.55 and DEM L204 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 X-Rays and Infrared: 0453.1-66.55 and DEM L204, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Supernova Remnants in X-Rays and Infrared: 0453.1-66.55 and DEM L204 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1022664