Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...324...27d&link_type=abstract
Astronomy and Astrophysics, v.324, p.27-31
Astronomy and Astrophysics
Astrophysics
15
Cosmic Microwave Background, Cosmology: Theory, Molecular Processes
Scientific paper
The luminescence process for proto-objects moving with a peculiar velocity at high redshift is considered. It is shown that some primordial molecules could produce low-frequency photons (which correspond to the rotational lines) by decaying high-frequency rovibration photons from the CBR. Due to the rather different numbers of these photons, a huge enhancement (relative to the pure reflection mechanism) of the emission line intensity from the proto-objects could occur at the appropriate wavelengths.
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