The Astrophysical Journal Letters (Jan 2023)

GOALS-JWST: NIRCam and MIRI Imaging of the Circumnuclear Starburst Ring in NGC 7469

  • Thomas Bohn,
  • Hanae Inami,
  • Tanio Diaz-Santos,
  • Lee Armus,
  • S. T. Linden,
  • Vivian U,
  • Jason Surace,
  • Kirsten L. Larson,
  • Aaron S. Evans,
  • Shunshi Hoshioka,
  • Thomas Lai,
  • Yiqing Song,
  • Joseph M. Mazzarella,
  • Loreto Barcos-Munoz,
  • Vassilis Charmandaris,
  • Justin H. Howell,
  • Anne M. Medling,
  • George C. Privon,
  • Jeffrey A. Rich,
  • Sabrina Stierwalt,
  • Susanne Aalto,
  • Torsten Böker,
  • Michael J. I. Brown,
  • Kazushi Iwasawa,
  • Matthew A. Malkan,
  • Paul P. van der Werf,
  • Philip Appleton,
  • Christopher C. Hayward,
  • Francisca Kemper,
  • David Law,
  • Jason Marshall,
  • Eric J. Murphy,
  • David Sanders

DOI
https://doi.org/10.3847/2041-8213/acab61
Journal volume & issue
Vol. 942, no. 2
p. L36

Abstract

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We present James Webb Space Telescope (JWST) imaging of NGC 7469 with the Near-Infrared Camera and the Mid-InfraRed Instrument. NGC 7469 is a nearby, z = 0.01627, luminous infrared galaxy that hosts both a Seyfert Type-1.5 nucleus and a circumnuclear starburst ring with a radius of ∼0.5 kpc. The new near-infrared (NIR) JWST imaging reveals 66 star-forming regions, 37 of which were not detected by Hubble Space Telescope (HST) observations. Twenty-eight of the 37 sources have very red NIR colors that indicate obscurations up to A _v ∼ 7 and a contribution of at least 25% from hot dust emission to the 4.4 μ m band. Their NIR colors are also consistent with young (<5 Myr) stellar populations and more than half of them are coincident with the mid-infrared (MIR) emission peaks. These younger, dusty star-forming regions account for ∼6% and ∼17% of the total 1.5 and 4.4 μ m luminosity of the starburst ring, respectively. Thanks to JWST, we find a significant number of young dusty sources that were previously unseen due to dust extinction. The newly identified 28 young sources are a significant increase compared to the number of HST-detected young sources (4–5). This makes the total percentage of the young population rise from ∼15% to 48%. These results illustrate the effectiveness of JWST in identifying and characterizing previously hidden star formation in the densest star-forming environments around active galactic nuclei (AGN).

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