Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-11-14
Astrophys.J.639:724-730,2006
Astronomy and Astrophysics
Astrophysics
7 pages, 4 figures. Accepted for publication by Astrophysical Journal
Scientific paper
10.1086/499576
In the Hubble Ultra Deep Field (HUDF) an abundance of galaxies is seen with a knot at one end plus an extended tail, resembling a tadpole. These "tadpole galaxies" appear dynamically unrelaxed--presumably in an early merging state--where tidal interactions likely created the distorted knot-plus-tail morphology. Here we systematically select tadpole galaxies from the HUDF and study their properties as a function of their photometric redshifts. In a companion HUDF variability study, Cohen et al. (2005) revealed a total of 45 variable objects believed to be Active Galactic Nuclei (AGN). Here we show that this faint AGN sample has no overlap with the tadpole galaxy sample, as predicted by theoretical work. The tadpole morphology--combined with the lack of overlap with the variable objects--supports the idea that these galaxies are in the process of an early-stage merger event, i.e., at a stage that likely precedes the "turn-on" of any AGN component and the onset of any point-source variability.
Cohen Seth H.
Hathi Nimish P.
Jansen Rolf A.
Ryan Russell E. Jr.
Straughn Amber N.
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