Numerical models for the dust in RCW 120
arXiv:1909.07150 · doi:10.1051/0004-6361/201935993
Abstract
The interstellar bubble RCW 120 seen around a type O runaway star is driven by the stellar wind and the ionising radiation emitted by the star. The boundary between the stellar wind and interstellar medium (ISM) is associated with the arc-shaped mid-infrared dust emission around the star within the HII region.
6 pages, 5 figures, 1 table, accepted for publication in A&A