Molecular Co(1-0) gas in the z ∼ 2 radio galaxy MRC0152-209

B. H C Emonts, I. Feain, M. Y. Mao, R. P. Norris, G. Miley, R. D. Ekers, M. Villar-Martín, H. J A Röttgering, E. M. Sadler, G. Rees, R. Morganti, D. J. Saikia, T. A. Oosterloo, J. B. Stevens, C. N. Tadhunter

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Abstract

We report the detection of molecular CO(1-0) gas in the high-z radio galaxy MRC0152-209 (z = 1.92) with the Australia Telescope Compact Array Broadband Backend (ATCA/CABB). This is the third known detection of CO(1-0) in a high-z radio galaxy to date. CO(1-0) is the most robust tracer of the overall molecular gas content (including the widespread, low-density, and sub-thermally excited component), hence observations of CO(1-0) are crucial for studying galaxy evolution in the early universe. We derive L′CO = 6.6 2.0 × 1010 K km s-1 pc2 for MRC0152-209, which is comparable to that derived from CO(1-0) observations of several high-z submillimeter and star-forming BzK galaxies. The CO(1-0) traces a total molecular hydrogen mass of = 5 × 1010x/0.8) M. MRC0152-209 is an infrared bright radio galaxy, in which a large reservoir of cold molecular gas has not (yet) been depleted by star formation or radio source feedback. Its compact radio source is reliably detected at 40 GHz and has a steep spectral index of α = -1.3 between 1.4 and 40 GHz (4-115 GHz in the galaxy's rest frame). MRC0152-209 is part of an ongoing systematic ATCA/CABB survey of CO(1-0) in high-z radio galaxies between 1.7 < z < 3.

Original languageEnglish
Article numberL25
Pages (from-to)1-5
Number of pages5
JournalAstrophysical Journal Letters
Volume734
Issue number1 PART 2
DOIs
Publication statusPublished - 10 Jun 2011
Externally publishedYes

Keywords

  • galaxies: active
  • galaxies: evolution
  • galaxies: high-redshift
  • galaxies: individual (MRC 0152-209)
  • galaxies: ISM
  • radio lines: ISM

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    Emonts, B. H. C., Feain, I., Mao, M. Y., Norris, R. P., Miley, G., Ekers, R. D., ... Tadhunter, C. N. (2011). Molecular Co(1-0) gas in the z ∼ 2 radio galaxy MRC0152-209. Astrophysical Journal Letters, 734(1 PART 2), 1-5. [L25]. https://doi.org/10.1088/2041-8205/734/1/L25