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Magnetic Field Uniformity Across the GF 9-2 YSO, L1082C Dense Core, and GF 9 Filamentary Dark Cloud

  • Authors: Dan P. Clemens, A. M. El Batal, C. Cerny, S. Kressy, G. Schroeder, and T. Pillai

2018 The Astrophysical Journal 867 79.

  • Provider: AAS Journals

Caption: Figure 2.

Inverted grayscale Mimir image of stacked K-band NIR observations of the L1082C core and GF 9-2 YSO covering the same field of view as delineated by the black square in Figure 1. SOFIA HAWC+ total 216 μm intensity contours are overlaid in black, spanning 20–260 MJy sr−1. The extent of the HAWC+ sampled region is shown as the magenta polygon. Colored circles identify stars that appear in Gaia Data Release 2 and have a parallax S/N greater than two, with colors identifying distance bins (red for closer than 0.5 kpc, green for 0.5–1.0 kpc, and blue for beyond 1.0 kpc).

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