Abstract
The growth of supermassive black holes appears to be driven by galaxy mergers, violent merger-free processes and/or 'secular' processes. In order to quantify the effects of secular evolution on black hole growth, we study a sample of active galactic nuclei (AGN) in galaxies with a calm formation history free of significant mergers, a population that heretofore has been difficult to locate. Here we present an initial sample of 13 AGN in massive (M ≳ 10M) bulgeless galaxies - which lack the classical bulges believed inevitably to result from mergers - selected from the Sloan Digital Sky Survey using visual classifications from Galaxy Zoo. Parametric morphological fitting confirms that the host galaxies lack classical bulges; any contributions from pseudo-bulges are very small (typically
| Original language | English |
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| Pages (from-to) | 2199-2211 |
| Number of pages | 13 |
| Journal | Monthly Notices of the Royal Astronomical Society (MNRAS) |
| Volume | 429 |
| Issue number | 3 |
| Early online date | 4 Jan 2013 |
| DOIs | |
| Publication status | Published - Mar 2013 |