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

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.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-000F-117D-F Version Permalink: http://hdl.handle.net/11858/00-001M-0000-000F-117E-D
Genre: Journal Article

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 Creators:
Cisternas, Mauricio, Author
Jahnke, Knud, Author
Bongiorno, Angela1, Author              
Inskip, Katherine J., Author
Impey, Chris D., Author
Koekemoer, Anton M., Author
Merloni, Andrea1, Author              
Salvato, Mara, Author
Trump, Jonathan R., Author
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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Language(s): eng - English
 Dates: 2011-11-01
 Publication Status: Published in print
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1088/2041-8205/741/1/L11
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Title: The Astrophysical Journal Letters
  Abbreviation : Astrophys. J. Lett.
Source Genre: Journal
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Pages: - Volume / Issue: 741 (1) Sequence Number: L11 Start / End Page: 1 - 6 Identifier: ISSN: 2041-8205