No More Active Galactic Nuclei in Clumpy Disks Than in Smooth Galaxies at z~2 in CANDELS / 3D-HST

Jonathan R. Trump,Guillermo Barro,Stéphanie Juneau,Benjamin J. Weiner,Bin Luo,Gabriel Brammer,Eric F. Bell,W. Niel Brandt,Avishai Dekel,Yicheng Guo,Philip F. Hopkins,David C. Koo,Dale D. Kocevski,Daniel H. McIntosh,Ivelina Momcheva,S. M. Faber,Henry C. Ferguson,Norman A. Grogin,Jeyhan Kartaltepe,Anton M. Koekemoer,Jennifer M. Lotz,Michael V. Maseda,Mark Mozena,Kirpal Nandra,David J. Rosario,Gregory R. Zeimann

No More Active Galactic Nuclei in Clumpy Disks Than in Smooth Galaxies at z~2 in CANDELS / 3D-HST

2014

We use CANDELS imaging, 3D-HST spectroscopy, and Chandra X-ray data to investigate if active galactic nuclei (AGNs) are preferentially fueled by violent disk instabilities funneling gas into galaxy centers at 1.3

Keywords:

spatially resolved
Astrophysics
Star formation
Active galactic nucleus
Galaxy
Spectroscopy
Gravitation
Population
Redshift
Physics

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