Is the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies?
We developed a hierarchical Bayesian model (HBM) to investigate how the presence of Seyfert activity relates to their environment, herein represented by the galaxy cluster mass, M200, and the normalized cluster centric distance, r/r200. We achieved this by constructing an unbiased sample of galaxies...
| Main Authors: | , , , , , , , , , |
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| Format: | Journal article |
| Published: |
Oxford University Press
2016
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