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Secular evolution and a non-evolving black-hole-to-galaxy mass ratio in the last 7 Gyr

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Bongiorno,  Angela
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4724

Merloni,  Andrea
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Cisternas, M., Jahnke, K., Bongiorno, A., Inskip, K. J., Impey, C. D., Koekemoer, A. M., et al. (2011). Secular evolution and a non-evolving black-hole-to-galaxy mass ratio in the last 7 Gyr. The Astrophysical Journal Letters, 741(1): L11, pp. 1-6. doi:10.1088/2041-8205/741/1/L11.


Cite as: http://hdl.handle.net/11858/00-001M-0000-000F-117D-F
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