... The most likely source of these photons originating so far, 100 kpc, from the quasar core is the cosmic microwavebackground. ... in the same way as PKS 0637-752: as inverse Compton scattering of the Cosmic Microwavebackground (Marshall et al, 2004 ...
... Cosmic MicrowaveBackground Radiation (CMBR). ... background temperature of 2.72 K. This corresponds to a peak wavelength that ... An Introduction to the Cosmic MicrowaveBackground Radiation (http://background ...
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Ссылки http://www.atnf.csiro.au/outreach/education/teachers/resources/CosmoCosmicEngine.pdf -- 577.5 Кб -- 22.01.2014 Похожие документы
... 1) The diffuse H emission as a tracer of the free-free foreground that contaminates the fluctuations in the cosmic microwavebackground radiation; (2) The H emission from galaxies as a measure of the formation rate of massive stars, both at low and high ...
... Sciama (1999) has pointed out that the local cloud population should also be detectable with future satellite missions (MAP and Planck) designed to study the Cosmic MicrowaveBackground. ...
... AMiBA: broadband heterodyne cosmic microwavebackground interferometry". ... The Yuan-Tseh Lee Array for microwavebackground anisotropy". ... WILSON, W. "Array for MicrowaveBackground Anisotropy: observations, data analysis ...
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Ссылки http://www.atnf.csiro.au/research/publications/ATNF_Publications_2009.pdf -- 85.2 Кб -- 03.03.2010 Похожие документы
... while simultaneously remaining consistent with measurements of the cosmic microwavebackground (CMB) anisotropies ... The fact that the cosmic microwavebackground (CMB) is smooth to 10-5 K on large scales (Smoot et al. 1992) tells us that the ...