CO J = 2-1 line emission in cluster galaxies at z ̃ 1

Fueling star formation in dense environments

Jeff Wagg, Alexandra Pope, Stacey Alberts, Lee Armus, Mark Brodwin, Robert S. Bussmann, Vandana Desai, Arjun Dey, Buell Tomasson Jannuzi, Emeric Le Floc'H, Jason Melbourne, Daniel Stern

Research output: Contribution to journalArticle

15 Citations (Scopus)

Abstract

We present observations of CO J = 2-1 line emission in infrared-luminous cluster galaxies at z 1 using the IRAM Plateau de Bure Interferometer. Our two primary targets are optically faint, dust-obscured galaxies (DOGs) found to lie within 2Mpc of the centers of two massive (>1014 M) galaxy clusters. CO line emission is not detected in either DOG. We calculate 3σ upper limits to the CO J = 2-1 line luminosities, L′CO < 6.08 × 109 and <6.63 × 109 Kkms -1pc2. Assuming a CO-to-H2 conversion factor derived for ultraluminous infrared galaxies in the local universe, this translates to limits on the cold molecular gas mass of and . Both DOGs exhibit mid-infrared continuum emission that follows a power law, suggesting that an active galactic nucleus (AGN) contributes to the dust heating. As such, estimates of the star formation efficiencies in these DOGs are uncertain. A third cluster member with an infrared luminosity, L IR < 7.4 × 1011 L, is serendipitously detected in CO J = 2-1 line emission in the field of one of the DOGs located roughly two virial radii away from the cluster center. The optical spectrum of this object suggests that it is likely an obscured AGN, and the measured CO line luminosity is L′CO = (1.94 ± 0.35) × 1010 Kkms -1pc2, which leads to an estimated cold molecular gas mass . A significant reservoir of molecular gas in a z 1 galaxy located away from the cluster center demonstrates that the fuel can exist to drive an increase in star formation and AGN activity at the outskirts of high-redshift clusters.

Original languageEnglish (US)
Article number91
JournalAstrophysical Journal
Volume752
Issue number2
DOIs
StatePublished - Jun 20 2012
Externally publishedYes

Fingerprint

refueling
star formation
galaxies
dust
molecular gases
active galactic nuclei
cold gas
luminosity
gas
interferometer
power law
plateau
heating
optical spectrum
plateaus
interferometers
universe
continuums
radii

Keywords

  • galaxies: clusters: general
  • galaxies: evolution
  • galaxies: formation
  • ISM: molecules

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Wagg, J., Pope, A., Alberts, S., Armus, L., Brodwin, M., Bussmann, R. S., ... Stern, D. (2012). CO J = 2-1 line emission in cluster galaxies at z ̃ 1: Fueling star formation in dense environments. Astrophysical Journal, 752(2), [91]. https://doi.org/10.1088/0004-637X/752/2/91

CO J = 2-1 line emission in cluster galaxies at z ̃ 1 : Fueling star formation in dense environments. / Wagg, Jeff; Pope, Alexandra; Alberts, Stacey; Armus, Lee; Brodwin, Mark; Bussmann, Robert S.; Desai, Vandana; Dey, Arjun; Jannuzi, Buell Tomasson; Le Floc'H, Emeric; Melbourne, Jason; Stern, Daniel.

In: Astrophysical Journal, Vol. 752, No. 2, 91, 20.06.2012.

Research output: Contribution to journalArticle

Wagg, J, Pope, A, Alberts, S, Armus, L, Brodwin, M, Bussmann, RS, Desai, V, Dey, A, Jannuzi, BT, Le Floc'H, E, Melbourne, J & Stern, D 2012, 'CO J = 2-1 line emission in cluster galaxies at z ̃ 1: Fueling star formation in dense environments', Astrophysical Journal, vol. 752, no. 2, 91. https://doi.org/10.1088/0004-637X/752/2/91
Wagg, Jeff ; Pope, Alexandra ; Alberts, Stacey ; Armus, Lee ; Brodwin, Mark ; Bussmann, Robert S. ; Desai, Vandana ; Dey, Arjun ; Jannuzi, Buell Tomasson ; Le Floc'H, Emeric ; Melbourne, Jason ; Stern, Daniel. / CO J = 2-1 line emission in cluster galaxies at z ̃ 1 : Fueling star formation in dense environments. In: Astrophysical Journal. 2012 ; Vol. 752, No. 2.
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abstract = "We present observations of CO J = 2-1 line emission in infrared-luminous cluster galaxies at z 1 using the IRAM Plateau de Bure Interferometer. Our two primary targets are optically faint, dust-obscured galaxies (DOGs) found to lie within 2Mpc of the centers of two massive (>1014 M) galaxy clusters. CO line emission is not detected in either DOG. We calculate 3σ upper limits to the CO J = 2-1 line luminosities, L′CO < 6.08 × 109 and <6.63 × 109 Kkms -1pc2. Assuming a CO-to-H2 conversion factor derived for ultraluminous infrared galaxies in the local universe, this translates to limits on the cold molecular gas mass of and . Both DOGs exhibit mid-infrared continuum emission that follows a power law, suggesting that an active galactic nucleus (AGN) contributes to the dust heating. As such, estimates of the star formation efficiencies in these DOGs are uncertain. A third cluster member with an infrared luminosity, L IR < 7.4 × 1011 L, is serendipitously detected in CO J = 2-1 line emission in the field of one of the DOGs located roughly two virial radii away from the cluster center. The optical spectrum of this object suggests that it is likely an obscured AGN, and the measured CO line luminosity is L′CO = (1.94 ± 0.35) × 1010 Kkms -1pc2, which leads to an estimated cold molecular gas mass . A significant reservoir of molecular gas in a z 1 galaxy located away from the cluster center demonstrates that the fuel can exist to drive an increase in star formation and AGN activity at the outskirts of high-redshift clusters.",
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