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Narrow-line Seyfert Galaxies. Connection between abundance and the large-scale structure

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, , Citation A A Ermash and B V Komberg 2014 J. Phys.: Conf. Ser. 572 012002 DOI 10.1088/1742-6596/572/1/012002

1742-6596/572/1/012002

Abstract

Utilizing methods, developed by the author the correlations between spatial concentrations of active nuclei (NLS and BLS) and concentration of galaxies of full uniform sample were obtained. Galaxies of this uniform sample trace the large-scale structure. We used SDSS DR 7 data. The correlations obtained are linear and the NLS/BLS ratio is constant. That leads to conclusion that amounts NLS and BLS are some fixed portion of all galaxies independent on the density of large-scale environment. In order to check validity of our results we also confirmed the well known result that fraction of red galaxies increases with density of environment. Also it was confirmed that this trend is more prominent for less massive galaxies.

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10.1088/1742-6596/572/1/012002