Diffuse X-ray Emission and Star Clusters in Nearby, Face-on Spiral Galaxies

Details Diffuse X-ray Emission and Star Clusters in Nearby, Face-on Spiral Galaxies Diffuse X-ray Emission and Star Clusters in Nearby, Face-on Spiral Galaxies

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21934630v&link_type=abstract

American Astronomical Society, AAS Meeting #219, #346.30

Astronomy and Astrophysics

Astronomy

Scientific paper

Supernovae or star clusters are expected to heat the interstellar
medium and drive material into a galaxy's halo. The X-ray emission of
nearby, edge-on spirals shows diffuse emission above their midplanes. For face-on spirals, we may expect a non-uniform distribution of emission if star clusters are important sources of energy. We describe the analyses and results of a study of the diffuse emission in several nearby, face-on spiral galaxies.

Affiliated with

Also associated with

No associations

Rating

Diffuse X-ray Emission and Star Clusters in Nearby, Face-on Spiral Galaxies 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 Diffuse X-ray Emission and Star Clusters in Nearby, Face-on Spiral Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Diffuse X-ray Emission and Star Clusters in Nearby, Face-on Spiral Galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1582040