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The Bolocam Galactic Plane Survey. XII. Distance Catalog Expansion Using Kinematic Isolation of Dense Molecular Cloud Structures with 13CO(1-0)

  • Authors: Timothy P. Ellsworth-Bowers, Erik Rosolowsky, Jason Glenn, Adam Ginsburg, Neal J. Evans II, Cara Battersby, Yancy L. Shirley, and Brian Svoboda

Ellsworth-Bowers et al. 2015 The Astrophysical Journal 799 29.

  • Provider: AAS Journals

Caption: Figure 7.

Example of DPDFpx construction from trigonometric parallax measurements. Left: Gaussians in parallax with μpx = 0.20 mas (μpx = 0.10 mas) and σpx = 0.03 mas are plotted in black (gray). The full-width error bars (i.e., μ ± σ) are shown in red (cyan). Middle: interpolation of the parallax functions onto a linear distance scale, where d =1/πs. The corresponding full-width error bars are shown in red (cyan). Right: size of the full-width distance error bar as a function of parallax measurement uncertainty and heliocentric distance. The curves shown represent the lower bound on the uncertainty (σπ = 0.005 mas), a typical value (σπ = 0.03 mas), and a poorly constrained parallax measurement (σπ = 0.10 mas). The red and cyan stars identify the examples at left, and the gray dashed line marks the 1:1 relationship.

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