The ISM properties and gas kinematics of a redshift 3 massive dusty star-forming galaxy.

@article{Leung2019TheIP,
  title={The ISM properties and gas kinematics of a redshift 3 massive dusty star-forming galaxy.},
  author={Tsz Kuk Daisy Leung and Dominik A. Riechers and Andrew Jordan Baker and Dave L. Clements and Asantha Cooray and Christopher C Hayward and Rob J. Ivison and Roberto Neri and Alain Omont and Ismael P'erez-Fournon and Douglas Scott and Julie L. Wardlow Cornell and Flatiron and Rutgers and Imperial College London and UC Irvine and Eso and Edinburgh and Iram and Institut d'Astrophysique de Paris and Instituto de Astrof'isica de Canarias and Universidad de la Laguna and University of British Columbia and Durham and Lancaster},
  journal={The Astrophysical Journal},
  year={2019},
  volume={871},
  pages={85}
}
  • Tsz Kuk Daisy Leung, Dominik A. Riechers, +22 authors Lancaster
  • Published 2019
  • Physics
  • The Astrophysical Journal
  • We present CO (J = 1 → 0 3 → 2 5 → 4 10 → 9) and 1.2 kpc resolution [C II] line observations of the dusty star-forming galaxy (SFG) HXMM05—carried out with the Karl G. Jansky Very Large Array, the Combined Array for Research in Millimeter-wave Astronomy, the Plateau de Bure Interferometer, and the Atacama Large Millimeter/submillimeter Array, measuring an unambiguous redshift of z = 2.9850 ± 0.0009. We find that HXMM05 is a hyperluminous infrared galaxy ({L}IR} = (4 ± 1) × 1013 L ⊙) with a… CONTINUE READING

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