NOEMA

We present a very deep CO(3–2) observation of a massive, gas-rich, main sequence, barred spiral galaxy at z ≈ 1.52. Our data were taken with the IRAM-NOEMA interferometer for a 12-antenna equivalent on-source integration time of ∼50 hours. We fit the major axis kinematics with the forward modeling of a rotating disk and subtracted the two-dimensional beam convolved best-fit model, which revealed signatures of planar noncircular motions in the residuals. The inferred in-plane radial velocities are remarkably high, of the order of ≈60 km/s. Direct comparisons with a high-resolution, simulated, gas-rich, barred galaxy, obtained with the moving mesh code <ns0:monospace>AREPO</ns0:monospace> and the <ns0:monospace>TNG</ns0:monospace> sub-grid model, show that the observed noncircular gas flows can be explained as radial flows driven by the central bar, with an inferred net inflow rate of the order of the star formation rate (SFR). Given the recent evidence for a higher-than-expected fraction of barred disk galaxies at cosmic noon, our results suggest that rapid gas inflows due to bars could be important evolutionary drivers for the dominant population of star-forming galaxies at the peak epoch of star and galaxy formation.

Authors

Publication Details

Journal
Springer Link (Chiba Institute of Technology)
Published
2025-12-19
DOI
https://doi.org/10.1051/0004-6361/202555430/pdf
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
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article

NOEMA

Juan M. Espejo Salcedo, Thorsten Naab, R. Davies, S. García‐Burillo et al.
Springer Link (Chiba Institute of Technology)
Galaxies: Formation, Evolution, Phenomena
article

NOEMA

Juan M. Espejo Salcedo, Thorsten Naab, R. Davies, S. García‐Burillo, C. Pulsoni, Rodrigo Herrera-Camus, Stijn Wuyts, A. Sternberg, Capucine Barfety, Sedona H. Price, DaiZhong Liu, Eleonora Parlanti, Letizia Scaloni, Yixian Cao, Minju Lee, Frank Eisenhauer, Jianhang Chen, Lilian L. Lee, Hannah Übler, Eckhard Sturm, Karl Schuster, Françoise Combes, Dieter Lutz, Alvio Renzini, Natascha M. Förster Schreiber, Stavros Pastras, Reinhard Genzel, Roberto Neri, Jean-Baptiste Jolly, Taro T. Shimizu, Andreas Burkert, Linda J. Tacconi, Volker Springel, Amit Nestor Shachar, Giulia Tozzi
article en

Abstract

We present a very deep CO(3–2) observation of a massive, gas-rich, main sequence, barred spiral galaxy at z ≈ 1.52. Our data were taken with the IRAM-NOEMA interferometer for a 12-antenna equivalent on-source integration time of ∼50 hours. We fit the major axis kinematics with the forward modeling of a rotating disk and subtracted the two-dimensional beam convolved best-fit model, which revealed signatures of planar noncircular motions in the residuals. The inferred in-plane radial velocities are remarkably high, of the order of ≈60 km/s. Direct comparisons with a high-resolution, simulated, gas-rich, barred galaxy, obtained with the moving mesh code <ns0:monospace>AREPO</ns0:monospace> and the <ns0:monospace>TNG</ns0:monospace> sub-grid model, show that the observed noncircular gas flows can be explained as radial flows driven by the central bar, with an inferred net inflow rate of the order of the star formation rate (SFR). Given the recent evidence for a higher-than-expected fraction of barred disk galaxies at cosmic noon, our results suggest that rapid gas inflows due to bars could be important evolutionary drivers for the dominant population of star-forming galaxies at the peak epoch of star and galaxy formation.

Springer Link (Chiba Institute of Technology)
Openalex Percentile: Top 29%
Galaxies: Formation, Evolution, Phenomena
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