Document Type

Article

Publication Date

8-1-2017

Publication Title

The Astrophysical Journal Letters

Abstract

We report the detection of CO(2–1) emission coincident with the brightest cluster galaxy (BCG) of the high- redshift galaxy cluster SpARCS1049+56, with the Redshift Search Receiver (RSR) on the Large Millimeter Telescope (LMT). We confirm a spectroscopic redshift for the gas of z = 1.7091 ± 0.0004, which is consistent with the systemic redshift of the cluster galaxies of z = 1.709. The line is well fit by a single-component Gaussian with an RSR-resolution-corrected FWHM of 569 ± 63kms−1. We see no evidence for multiple velocity components in the gas, as might be expected from the multiple image components seen in near-infrared imaging with the Hubble Space Telescope. We measure the integrated flux of the line to be 3.6 ± 0.3 Jy km s−1, and using aCO = 0.8 Me (K km s−1 pc2)−1, we estimate a total molecular gas mass of 1.1 ± 0.1 × 1011 Me and a MH2/Må ∼ 0.4. This is the largest gas reservoir detected in a BCG above z > 1 to date. Given the infrared- estimated star formation rate of 860 ± 130 Me yr−1, this corresponds to a gas depletion timescale of ∼0.1 Gyr. We discuss several possible mechanisms for depositing such a large gas reservoir to the cluster center—e.g., a cooling flow, a major galaxy–galaxy merger, or the stripping of gas from several galaxies—but conclude that these LMT data are not sufficient to differentiate between them.

Keywords

galaxies: clusters, individual (SpARCS1049+56), galaxies: evolution, galaxies: starburst, ISM: molecules

Volume

844

Issue

L17

DOI

doi.org/10.3847/2041-8213/aa7749

Rights

© 2017. The American Astronomical Society. All rights reserved.

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