The power source of very luminous infrared galaxies.
Seven very luminous galaxies were examined to determine the contribution of active nuclei to their luminosity, the nature of their stellar population, and the validity of previous measurements of their H₂ content. Spectra of the 2.3 μm bands of CO were used to measure the stellar velocity dispersion...
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| Language: | en |
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The University of Arizona.
1995
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| Online Access: | http://hdl.handle.net/10150/187129 |