STELLAR AND BLACK HOLE MASS DENSITIES AS EMPIRICAL TRACERS OF CO-EVOLUTION SHOW LOCK-STEP GROWTH SINCE Z ∼ 3
At redshifts beyond z similar to 1, measuring the black hole (BH) galaxy relations proves to be a difficult task. The bright light of the active galactic nuclei aggravates the deconvolution of BH and galaxy properties. However, high-redshift data on these relations are vital to understand the ways i...
| Main Authors: | , , |
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| Other Authors: | |
| Language: | en |
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IOP PUBLISHING LTD
2016
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| Online Access: | http://hdl.handle.net/10150/621377 http://arizona.openrepository.com/arizona/handle/10150/621377 |