no code implementations • 22 Jan 2021 • Jeremy Chastenet, Karin Sandstrom, I-Da Chiang, Brandon S. Hensley, Bruce T. Draine, Karl D. Gordon, Eric W. Koch, Adam K. Leroy, Dyas Utomo, Thomas G. Williams
We show that renormalizing the models to match the same Milky Way high latitude cirrus spectrum and abundance constraints can reduce the dust mass differences between models and bring the total dust mass below the maximum estimate at all radii.
Astrophysics of Galaxies
