 When formed through dynamical interactions, stellarmass binary black holes may retain eccentric orbits ($e>0.1$ at 10\,Hz) detectable by groundbased gravitationalwave detectors. Eccentricity can therefore be used to differentiate dynamicallyformed binaries from isolated binary black hole mergers. Current templatebased gravitationalwave searches do not use waveform models associated to eccentric orbits, rendering the search less efficient to eccentric binary systems. Here we present results of a search for binary black hole mergers that inspiral in eccentric orbits using data from the first and second observing runs (O1 and O2) of Advanced LIGO and Advanced Virgo. \add{We carried out the search with the coherent WaveBurst algorithm, which uses minimal assumptions on the signal morphology and does not rely on binary waveform templates.} We show that it is sensitive to binary mergers with a detection range that is weakly dependent on eccentricity for all bound systems. Our search did not identify any new binary merger candidates. We interpret these results in light of eccentric binary formation models. \add{We rule out formation channels with rates $\gtrsim100$\,Gpc$^{3}$\,yr$^{1}$ for $e>0.1$ assuming a black hole mass spectrum with powerlaw index $\lesssim2$.

 paper (eBBH_O1_O2.pdf, 358.7 kB)
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