1. Magnetic Field Uniformity Across the GF 9-2 YSO, L1082C Dense Core, and GF 9 Filamentary Dark Cloud
- Author
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A. M. El-Batal, C. Cerny, Dan P. Clemens, T. Pillai, S. Kressy, and G. Schroeder
- Subjects
Physics ,010504 meteorology & atmospheric sciences ,Data products ,business.industry ,Stratospheric Observatory for Infrared Astronomy ,Member states ,Library science ,FOS: Physical sciences ,Astronomy and Astrophysics ,Cloud computing ,01 natural sciences ,Astrophysics - Astrophysics of Galaxies ,Space and Planetary Science ,Observatory ,Astrophysics of Galaxies (astro-ph.GA) ,0103 physical sciences ,business ,Space research ,Astrophysics - Instrumentation and Methods for Astrophysics ,010303 astronomy & astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,0105 earth and related environmental sciences ,Dense core - Abstract
The orientation of the magnetic field (B-field) in the filamentary dark cloud GF 9 was traced from the periphery of the cloud into the L1082C dense core that contains the low-mass, low-luminosity Class 0 young stellar object (YSO) GF 9-2 (IRAS 20503+6006). This was done using SOFIA HAWC+ dust thermal emission polarimetry (TEP) at 216 um in combination with Mimir near-infrared background starlight polarimetry (BSP) conducted at H-band (1.6 um) and K-band (2.2 um). These observations were augmented with published I-band (0.77 um) BSP and Planck 850 um TEP to probe B-field orientations with offset from the YSO in a range spanning 6000 AU to 3 pc. No strong B-field orientation change with offset was found, indicating remarkable uniformity of the B-field from the cloud edge to the YSO environs. This finding disagrees with weak-field models of cloud core and YSO formation. The continuity of inferred B-field orientations for both TEP and BSP probes is strong evidence that both are sampling a common B-field that uniformly threads the cloud, core, and YSO region. Bayesian analysis of Gaia DR2 stars matched to the Mimir BSP stars finds a distance to GF 9 of 270 +/- 10 pc. No strong wavelength dependence of B-field orientation angle was found, contrary to previous claims., 18 pages, 6 figures ApJ, accepted
- Published
- 2018