Abstract
We present evidence of a dual active galactic nucleus (AGN) within an early-type galaxy at z = 0.709 in the extended Groth strip. The galaxy lies on the red sequence, with absolute magnitude MB = -21.0 (AB, with h = 0.7) and rest-frame color U - B = 1.38. Its optical spectrum shows strong, double-peaked [O III ] emission lines and weak Hβ emission, with Seyfert-like line ratios. The two narrow peaks are separated by 630 km s -1 in velocity and arise from two distinct regions, spatially resolved in the DEIMOS spectrum, with a projected physical separation of 1.2 kpc. HST ACS imaging shows an early-type (E/S0) galaxy with hints of disturbed structure, consistent with the remnant of a dissipationless merger. Multiwavelength photometric information from the AEGIS consortium confirms the identification of a dust-obscured AGN in an early-type galaxy, with detections in X-ray, optical, infrared, and radio wave bands. These data are most readily explained as a single galaxy harboring two AGNs-the first such system to be observed in an otherwise typical early-type galaxy.
Original language | English (US) |
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Pages (from-to) | L23-L26 |
Journal | Astrophysical Journal |
Volume | 660 |
Issue number | 1 II |
DOIs | |
State | Published - May 1 2007 |
Externally published | Yes |
Keywords
- Galaxies: active
- Galaxies: nuclei
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science