Chandra/ATCA Observations of the Large Magellanic Cloud Supernova Remnants N103B and N132D

Details Chandra/ATCA Observations of the Large Magellanic Cloud Supernova Remnants N103B and N132D Chandra/ATCA Observations of the Large Magellanic Cloud Supernova Remnants N103B and N132D

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...19912605p&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #126.05; Bulletin of the American Astronomical Society, Vol. 33, p.1489

Astronomy and Astrophysics

Astronomy

Scientific paper

In order to search for non-thermal X-ray emission from the Large Magellanic Cloud supernova remnants N103B and N132D, we have analyzed Chandra observations of these remnants and compared them to radio observations made using the Australia Telescope Compact Array (ATCA). We have extracted Advanced CCD Imaging Spectrometer (ACIS) spectra from regions in both remnants which are coincident with radio emission, and compared these against spectra taken from regions which are devoid of radio emission. Initial results and preliminary conclusions will be presented.

Affiliated with

Also associated with

No associations

Rating

Chandra/ATCA Observations of the Large Magellanic Cloud Supernova Remnants N103B and N132D 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 Chandra/ATCA Observations of the Large Magellanic Cloud Supernova Remnants N103B and N132D, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chandra/ATCA Observations of the Large Magellanic Cloud Supernova Remnants N103B and N132D will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1236283