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Much can be learned from detailed spectral studies (see spectroscopy) of the emission from accretion disks.
Even before they first detected the emission from neutral hydrogen in 1951, astronomers were aware of interstellar gas.
The emission from the disk displays such relativistic effects as gravitational redshift, in which the wavelength of the emitted light is shifted to longer wavelengths.
The emission from the non-Kasha state is possible.
This herringbone forming should affect the emission from the nanocrystals.
Parallel resonances can amplify the emission from individual turbines.
This is the reason that the emission from DBPPV and the emission from the ZnO are not observed in the DB ZnO devices.
The emission into the public grid is at most 45 times the emission from one turbine, or 15 times the emission from the three turbines.
The approach is validated in calculations of the emission from clean copper and silver surfaces.
The emission from the nicotinamide ring of NADH is used as a marker of structural transformations.
They are assigned to the emission from H- and J-aggregates and monomers.
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