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The fluctuations that we see in the CMBR most likely are: Group of answer choices due to difficulties with the detectors used to measure it
The fluctuations that we see in the CMBR most likely are: Group of answer choices due to difficulties with the detectors used to measure it due to the great distance to the CMBR due to how far back in the past the CMBR is the seeds of the stars and eventually the galaxies
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Light Scattering By Small Particles (Dover Books On Physics)
Authors: H. C. Van De Hulst Page
Corrected Edition
0486642283, 9780486642284
