Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1780197 | New Astronomy Reviews | 2007 | 13 Pages |
Abstract
S-Z polarization levels and patterns strongly depend on the non-uniform distributions of intracluster gas and on peculiar and internal velocities. We have therefore calculated the patterns of two polarization components that are produced when the CMB is doubly scattered in a simulated cluster. These are found to be very different than the patterns calculated based on spherical clusters with uniform structure and simplified gas distribution.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Y. Rephaeli, S. Sadeh, M. Shimon,