SOFIA/HAWC+ Far-infrared Polarimetric Large-area CMZ Exploration Survey. III. Full Survey Data Set

Details

• Journal Title:
  The Astrophysical Journal
• Personal Author:
  Paré, Dylan ; Butterfield, Natalie O. ; Chuss, David T. ; Guerra, Jordan A. ; Iuliano, Jeffrey Inara ; Karpovich, Kaitlyn ; Morris, Mark R. ; Wollack, Edward J.
• NOAA Program & Office:
  CIRES (Cooperative Institute for Research in Environmental Sciences)
• Description:
  We present the second data release (DR2) of the Far-InfraREd Polarimetric Large-Area CMZ Exploration (FIREPLACE) survey. This survey utilized the Stratospheric Observatory for Infrared Astronomy High-resolution Airborne Wideband Camera plus instrument at 214 μm (E band) at a resolution of 19.″6 to observe thermal polarized dust emission throughout the Central Molecular Zone (CMZ). DR2 consists of observations obtained in 2022 covering the region of the CMZ extending from the Brick to the Sgr C molecular clouds (corresponding to a 1° × 0.°75 region of the sky). We combine DR2 with the first FIREPLACE data release (DR1) to obtain full coverage of the CMZ (a 1.°5 × 0.°75 region of the sky). After applying total and polarized intensity significance cuts on the full FIREPLACE data set, we obtain ∼64,000 Nyquist-sampled polarization pseudovectors. The distribution of polarization pseudovectors confirms a bimodal distribution in the CMZ magnetic field orientations, recovering field components that are oriented predominantly parallel or perpendicular to the Galactic plane. This distribution of orientations is similar to what was observed in DR1 and other studies. We also inspect the magnetic fields toward a set of prominent CMZ molecular clouds (the Brick, Three Little Pigs, 50 and 20 km s−1 clouds, circumnuclear disk, CO 0.02-0.02, and Sgr C), revealing spatially varying magnetic fields having orientations that generally trace the total intensity morphologies of the clouds. We find evidence that compression from stellar winds and shear from tidal forces are prominent mechanisms influencing the structure of the magnetic fields.
• Source:
  The Astrophysical Journal, 969(2), 150
• DOI:
  https://doi.org/10.3847/1538-4357/ad4462
• ISSN:
  0004-637X ; 1538-4357
• Format:
  pdf
• Publisher:
  American Astronomical Society
• Document Type:
  Journal Article
• License:
  https://creativecommons.org/licenses/by/4.0/
• Rights Information:
  CC BY
• Compliance:
  Library
• Main Document Checksum:
  urn:sha-512:72f4552cfe24c81482ea00e60f40bb81b9193ecb305549507b1bf2ebe4e9a63e7056f9a16aadba1ba1d71d2dfb363fd932085dace81dd39377d8d0f88e5736c7
• Download URL:
  https://repository.library.noaa.gov/view/noaa/69698/noaa_69698_DS1.pdf
• File Type:
  [PDF - 6.85 MB ]