Non-thermal Emission in Clusters of Galaxies

Details Non-thermal Emission in Clusters of Galaxies Non-thermal Emission in Clusters of Galaxies

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.294...37f&link_type=abstract

Astrophysics and Space Science, Volume 294, Issue 1-2, pp. 37-43

Astronomy and Astrophysics

Astrophysics

11

Clusters Of Galaxies: Non-Thermal Emission

Scientific paper

The most evident signature for the presence of non-thermal elements (magnetic fields and relativistic electrons) in clusters of galaxies is given by the presence of diffuse radio regionspresent so far in a limited number of objects. We review the recent discoveries of new spectral components by EUVE and BeppoSAX in the spectra of some clusters of galaxies that allow to better determine the non-thermalquantities by relating radio and X-ray data.

Affiliated with

Also associated with

No associations

Rating

Non-thermal Emission in Clusters of 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 Non-thermal Emission in Clusters of Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-thermal Emission in Clusters of Galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1008925