Violent Quenching: Molecular Gas Blown to 1000 km s−1 during a Major Merger
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Issue Date
2018-08-23Author
Geach, James E.
Tremonti, Christy
Diamond-Stanic, A. M.
Sell, Paul H.
Kepley, Amanda
Coil, Alison L.
Rudnick, Gregory H.
Hickox, Ryan C.
Moustakas, John
Yang, Yujin
Publisher
American Astronomical Society
Type
Article
Article Version
Scholarly/refereed, publisher version
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We present Atacama Large Millimeter/submillimeter Array observations of a massive (${M}_{\star }\approx {10}^{11}\,{M}_{\odot }$) compact (${r}_{{\rm{e}},\mathrm{UV}}\approx 100$ pc) merger remnant at z = 0.66 that is driving a 1000 km s−1 outflow of cool gas, with no observational trace of an active galactic nucleus (AGN). We resolve molecular gas on scales of approximately 1–2 kpc, and our main finding is the discovery of a wing of blueshifted CO J(2 → 1) emission out to −1000 km s−1 relative to the stars. We argue that this is the molecular component of a multiphase outflow, expelled from the central starburst within the past 5 Myr through stellar feedback, although we cannot rule out previous AGN activity as a launching mechanism. If the latter is true, then this is an example of a relic multiphase AGN outflow. We estimate a molecular mass outflow rate of approximately 300 M ⊙ yr−1, or about one third of the 10 Myr-averaged star formation rate. This system epitomizes the multiphase "blowout" episode following a dissipational major merger—a process that has violently quenched central star formation and supermassive black hole growth.
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Citation
Geach, J. E., Tremonti, C., Diamond-Stanic, A. M., Sell, P. H., Kepley, A. A., Coil, A. L., ... & Yang, Y. (2018). Violent Quenching: Molecular Gas Blown to 1000 km s− 1 during a Major Merger. The Astrophysical Journal Letters, 864(1), L1.
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