A Study of 90 GHz Dust Emissivity on Molecular Cloud and Filament Scales
- Autor(en)
- Ian Lowe, Brian Mason, Tanay Bhandarkar, S. E. Clark, Mark Devlin, Simon R. Dicker, Shannon M. Duff, Rachel Friesen, Alvaro Hacar, Brandon Hensley, Tony Mroczkowski, Sigurd Naess, Charles Romero, Sarah Sadavoy, Maria Salatino, Craig Sarazin, John Orlowski-Scherer, Alessandro Schillaci, Jonathan Sievers, Thomas Stanke, Amelia Stutz, Zhilei Xu
- Abstrakt
Recent observations from the MUSTANG2 instrument on the Green Bank Telescope have revealed evidence of enhanced long-wavelength emission in the dust spectral energy distribution (SED) in the Orion Molecular Cloud (OMC) 2/3 filament on 25″ (0.1 pc) scales. Here we present a measurement of the SED on larger spatial scales (map size 0.°5-3° or 3-20 pc), at somewhat lower resolution (120″, corresponding to 0.25 pc at 400 pc) using data from the Herschel satellite and Atacama Cosmology Telescope (ACT). We then extend the 120″-scale investigation to other regions covered in the Herschel Gould Belt Survey (HGBS), specifically the dense filaments in the southerly regions of Orion A, Orion B, and Serpens-S. Our data set in aggregate covers approximately 10 deg2, with continuum photometry spanning from 160 μm to 3 mm. These OMC 2/3 data display excess emission at 3 mm, though less (10.9% excess) than what is seen at higher resolution. Strikingly, we find that the enhancement is present even more strongly in the other filaments we targeted, with an average excess of 42.4% and 30/46 slices showing an inconsistency with the modified blackbody to at least 4σ. Applying this analysis to the other targeted regions, we lay the groundwork for future high-resolution analyses. Additionally, we also consider a two-component dust model motivated by Planck results and an amorphous grain dust model. While both of these have been proposed to explain deviations in emission from a generic modified blackbody, we find that they have significant drawbacks, requiring many spectral points or lacking experimental data coverage.
- Organisation(en)
- Institut für Astrophysik
- Externe Organisation(en)
- University of Pennsylvania, National Radio Astronomy Observatory, Charlottesville, Princeton University, U.S. Department of Commerce, University of Toronto, European Southern Observatory (Germany), Flatiron Institute, National Radio Astronomy Observatory, Green Bank, Queen’s University, Kavli Institute for Particle Astrophysics and Cosmology, University of Virginia, California Institute of Technology (Caltech), McGill University, Universidad de Concepción, Massachusetts Institute of Technology
- Journal
- The Astrophysical Journal
- Band
- 929
- ISSN
- 0004-637X
- DOI
- https://doi.org/10.3847/1538-4357/ac5d4f
- Publikationsdatum
- 04-2022
- Peer-reviewed
- Ja
- ÖFOS 2012
- 103004 Astrophysik, 103003 Astronomie
- ASJC Scopus Sachgebiete
- Astronomy and Astrophysics, Space and Planetary Science
- Link zum Portal
- https://ucrisportal.univie.ac.at/de/publications/f272d29d-e823-4925-a89a-bbba6d723c1d