[Previous] | [Session 2] | [Next]
E. De Filippis, M.W. Bautz (MIT), M. Sereno, G. Longo (Universita' di Napoli, Federico II)
For many years SZ and X-ray data of galaxy clusters have been used in conjunction in order to infer fundamental cosmological informations. Results from WMAP, combined with other astronomical data, have recently enabled accurate testing of cosmological models and constrained the geometry of the universe.
Using the cosmology implied from WMAP, we are using a
combined X-ray and SZ analysis to obtain detailed
informations on cluster morphologies: we are able to measure
their shapes, elongation along the line of sight and
inclination respect to it. If also strong lensing data are
available, the need for a preassumption on cosmology ceases
and both cosmology and detailed morphology can be computed
for a cluster at the same time. In the last years Chandra
has provided unprecedented detailed images of the 2D
projected appearance of galaxy clusters, but we still know
so little on how and how much this is affected by projection
effects. Detailed informations on the three dimensional
geometry of galaxy clusters, are of fundamental importance
for a better understanding of their dynamical state, which
will allow a more correct determination of the spectral
parameters and mass distribution. We are applying this
procedure to a sample of clusters spanning a large redshift
range (0.02 The author(s) of this abstract have provided an email address
for comments about the abstract:
bdf@space.mit.edu
[Previous] |
[Session 2] |
[Next]
Bulletin of the American Astronomical Society, 36 #3
© 2004. The American Astronomical Soceity.