X-Ray Emission Mechanisms and Evolution of Superbubbles

Details X-Ray Emission Mechanisms and Evolution of Superbubbles X-Ray Emission Mechanisms and Evolution of Superbubbles

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cxo..prop.1033o&link_type=abstract

Chandra Proposal ID #03910326

Physics

Chandra Proposal Id #03910326

Scientific paper

We propose Chandra ACIS observations of four young superbubbles generated by stellar winds and supernovae of OB associations in the Large Magellanic Cloud. The imaging data will resolve the structure of the X-ray emission, allowing us to discriminate between the three principal models for superbubble X-ray emission. Since the X-ray luminosity is the most direct probe of the superbubble energy budgets, these data will strongly constrain models for superbubble evolution and resulting consequences for the multiphase ISM and galaxy evolution.

Affiliated with

Also associated with

No associations

Rating

X-Ray Emission Mechanisms and Evolution of Superbubbles 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 X-Ray Emission Mechanisms and Evolution of Superbubbles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-Ray Emission Mechanisms and Evolution of Superbubbles will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1488777