What is it about?

We employed a hierarchical Bayesian model​ to exploit the environmental effects of surrounding galaxies in the level of fuel for a supermassive black hole in the center of galaxies.

Featured Image

Read the Original

This page is a summary of: Is the cluster environment quenching the Seyfert activity in elliptical and spiral galaxies?, Monthly Notices of the Royal Astronomical Society, June 2016, Oxford University Press (OUP),
DOI: 10.1093/mnras/stw1459.
You can read the full text:

Read

Contributors

The following have contributed to this page