Image Details
Caption: Figure 19.
Posterior distributions from Bayesian analysis for I − P relation. The black lines delineate the 68% (1σ) highest-density interval (HDI). α is constrained to be significantly less than 1 with ﹩{0.36}_{-0.02}^{+0.03}﹩, suggesting that aligned dust grains are present within SDC13.
© 2022. The Author(s). Published by the American Astronomical Society.