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Interstellar Polarization Survey. V. Galactic Magnetic Field Tomography of the Spiral Arms Using Optical and Near-infrared Starlight Polarization

  • Authors: Y. Angarita, M. J. F. Versteeg, M. Haverkorn, V. Pelgrims, C. V. Rodrigues, A. M. Magalhães, R. Santos-Lima, Koji S. Kawabata

Y. Angarita et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 15.

GMM results with optical (the two left columns) and NIR (the two right columns) polarization in C5 (top), C45 (middle), and C50 (bottom). The first and third columns are the group separations in normalized qu space. The ellipses represent the Gaussian components. The second and fourth columns are the group membership probability as a function of photogeometric distance. The colors correspond to the components of Figures 8 10.

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