- Abstract:
-
We use data from the Sloan Digital Sky Survey and visual classifications of morphology from the Galaxy Zoo project to study black hole growth in the nearby Universe (z < 0.05) and to break down the AGN host galaxy population by color, stellar mass and morphology. We find that black hole growth at luminosities L_OIII >1E40 erg/s in early- and late-type galaxies is fundamentally different. AGN host galaxies as a population have a broad range of stellar masses (1E10-1E11 Msun), reside in t...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1088/0004-637X/711/1/284
-
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- Publisher:
- Institute of Physics Publishing
- Journal:
- ASTROPHYSICAL JOURNAL
- Volume:
- 711
- Issue:
- 1
- Pages:
- 284-302
- Publication date:
- 2010-01-18
- DOI:
- EISSN:
-
1538-4357
- ISSN:
-
0004-637X
- URN:
-
uuid:38b3abb6-39cb-4ba7-8b58-085d6346ef20
- Source identifiers:
-
161451
- Local pid:
- pubs:161451
- Language:
- English
- Keywords:
- Copyright date:
- 2010
- Notes:
-
22 pages, 12 figures, 3 tables. Accepted for publication in the
Astrophysical Journal. A version with full-resolution figures is available at
http://www.astro.yale.edu/ks57/papers/Schawinski.GZAGNhostgalaxies.2010.pdf
Journal article
Galaxy Zoo: The fundamentally different co-evolution of supermassive black holes and their early- and late-type host galaxies
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