We propose here XMM observations of Abell 1882; the first massive nearby clusterof galaxies observed by the SDSS. The region surrounding Abell 1882 is complexin the optical and X--ray wavelengths. In the optical, the main cluster core isextended with a bi-modal redshift distribution. However, the redshift histogramdoes not resemble typical merger scenarios. On the other hand, the peak X--rayemission is significantly offset from the galaxy concentration, indicative of amerging system. We will propose a detailed physical model for this system usinga combination of X--ray, optical data with new hydro/N--body simulations. Such amodel is essential for determining the roles of different physical mechanisms(e.g. turbulence, ram pressure, dissipation) on galaxy formation and evolution.
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2003-02-08T01:12:46Z/2003-02-08T07:45:33Z
Version
17.56_20190403_1200
Mission Description
The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
European Space Agency, Dr Chris Miller, 2004, 'A Multiwavelength Study of the Cosmic Web', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-8q6hoz1
