The Astrophysical Journal Letters (Jan 2022)

GOALS-JWST: Unveiling Dusty Compact Sources in the Merging Galaxy IIZw096

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

DOI
https://doi.org/10.3847/2041-8213/ac9389
Journal volume & issue
Vol. 940, no. 1
p. L6

Abstract

Read online

We have used the Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) to obtain the first spatially resolved, mid-infrared images of IIZw096, a merging luminous infrared galaxy (LIRG) at z = 0.036. Previous observations with the Spitzer Space Telescope suggested that the vast majority of the total IR luminosity ( L _IR ) of the system originated from a small region outside of the two merging nuclei. New observations with JWST/MIRI now allow an accurate measurement of the location and luminosity density of the source that is responsible for the bulk of the IR emission. We estimate that 40%–70% of the IR bolometric luminosity, or 3–5 × 10 ^11 L _⊙ , arises from a source no larger than 175 pc in radius, suggesting a luminosity density of at least 3–5 × 10 ^12 L _⊙ kpc ^−2 . In addition, we detect 11 other star-forming sources, five of which were previously unknown. The MIRI F1500W/F560W colors of most of these sources, including the source responsible for the bulk of the far-IR emission, are much redder than the nuclei of local LIRGs. These observations reveal the power of JWST to disentangle the complex regions at the hearts of merging, dusty galaxies.

Keywords