A

PRUSSIC

Astronomy and Astrophysics, vol. 667, pp. A70

Abstract

Dusty star-forming galaxies (DSFGs) at redshiftz ≥ 1 are among the most vigorously star-forming galaxies in the Universe. However, their dense (≥105cm−3) gas phase – typically traced by HCN(1–0) – remains almost entirely unexplored: only two DSFGs have been detected in HCN(1–0) to date. We present the results of aKarl G. JanskyVery Large Array survey of theJ = 1–0 transition of HCN, HCO+, and HNC(1–0) in six strongly lensed DSFGs atz = 2.5 − 3.3, effectively doubling the number of DSFGs with deep observations of these lines. We detect HCN(1–0) emission in one source (J1202+5354, 4.6σ), with a tentative HCO+(1–0) detection in another (J1609+6045, 3.3σ). Spectral stacking yields strict upper limits on the HCN/FIR (≤3.6 × 10−4) and HCN/CO(1–0) ratios (≤0.045). The inferred HCN/FIR ratios (a proxy for the star-formation efficiency) are consistent with those inz ∼ 0 far-infrared-luminous starbursts. However, the HCN/CO ratios – a proxy for the dense-gas fraction – are a factor of a few lower than suggested by the two previous DSFG detections. Our results imply that most DSFGs have low dense-gas fractions. A comparison with theoretical models of star-forming galaxies indicates that the bulk of gas in DSFGs is at lower densities (≈102cm−3), similar to ‘normal’ star-forming galaxies, rather than ultraluminous starbursts.

Authors 9

  1. Leiden University · Leiden Observatory · Delft University of Technology

    Affiliation as printed

    Faculty of Electrical Engineering, Mathematics and Computer Science, Delft University of Technology, Delft, The Netherlands

    Leiden Observatory, Leiden University, Niels Bohrweg 2, 2333 CA, Leiden, The Netherlands

  2. Leiden University · Leiden Observatory

    Affiliation as printed

    Leiden Observatory, Leiden University, Niels Bohrweg 2, 2333 CA, Leiden, The Netherlands

  3. DTU Space · University College London · Technical University of Denmark

    Affiliation as printed

    Cosmic Dawn Center (DAWN), København, Denmark

    DTU-Space, Technical University of Denmark, Elektrovej 327, 2800 Kgs. Lyngby, Denmark

    Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, UK

  4. University of Cologne

    Affiliation as printed

    I. Physikalisches Institut, Universität zu Köln, Zülpicher Strasse 77, 50937 Köln, Germany

  5. Centro de Astrobiología

    Affiliation as printed

    Centro de Astrobiología (CAB), CSIC-INTA, Cra. de Ajalvir Km. 4, 28850 Torrejón de Ardoz, Madrid, Spain

  6. Leiden University · European Southern Observatory · Leiden Observatory

    Affiliation as printed

    European Southern Observatory, Karl-Schwarzschild-Straße 2, 85748 Garching bei München, Germany

    Leiden Observatory, Leiden University, Niels Bohrweg 2, 2333 CA, Leiden, The Netherlands

  7. Max Planck Institute for Astronomy

    Affiliation as printed

    Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany

  8. SKA Observatory

    Affiliation as printed

    SKA Observatory, Lower Withington Maccleseld, Cheshire, SK11 9FT, UK

  9. Leiden University · Leiden Observatory

    Affiliation as printed

    Leiden Observatory, Leiden University, Niels Bohrweg 2, 2333 CA, Leiden, The Netherlands

Cited by 19 stored of 20

19 results

No patents citing this paper on Lens.org (checked 2026-10-11).

References 163