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• W3100014383 abstract "We present Atacama Large Millimeter/submillimeter Array measurements of the `Cosmic Seagull', a strongly magnified galaxy at z=2.7779 behind the Bullet Cluster. We report CO(3-2) and continuum 344~$mu$m (rest-frame) data at one of the highest differential magnifications ever recorded at submillimeter wavelengths ($mu$ up to ~50), facilitating a characterization of the kinematics of a rotational curve in great detail (at ~620 pc resolution in the source plane). We find no evidence for a decreasing rotation curve, from which we derive a dynamical mass of ($6.3pm0.7)times10^{10} M_{odot}$ within $r = 2.6pm0.1$ kpc. The discovery of a third, unpredicted, image provides key information for a future improvement of the lensing modeling of the Bullet Cluster and allows a measure of the stellar mass, $1.6^{+1.9}_{-0.86}times10^{10} M_{odot}$, unaffected by strong differential magnification. The baryonic mass is is expected to be dominated by the molecular gas content ($f_{gas} leq 80 pm 20$ %) based on an $M_{H_2}$ mass estimated from the difference between dynamical and stellar masses. The star formation rate is estimated via the spectral energy distribution ($SFR = 190 pm 10 M_{odot}/yr$), implying a molecular gas depletion time of $0.25pm0.08$ Gyr." @default.
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• W3100014383 date "2018-08-14" @default.
• W3100014383 modified "2023-10-03" @default.
• W3100014383 title "The “Cosmic Seagull”: A Highly Magnified Disk-like Galaxy at z ≃ 2.8 behind the Bullet Cluster" @default.
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• W3100014383 doi "https://doi.org/10.3847/2041-8213/aad6de" @default.
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