Resolved spectral variations of the centimetre-wavelength continuum from the rho Oph W photo-dissociation-region

no code implementations • 1 Oct 2020 • Simon Casassus, Matias Vidal, Carla Arce-Tord, Clive Dickinson, Glenn J. White, Michael Burton, Balthasar Indermuehle, Brandon Hensley

The EME is particularly bright in the regions of the rho Ophiuchi molecular cloud (rho Oph) that surround the earliest type star in the complex, HD 147889, where the peak signal stems from the filament known as the rho Oph-W PDR.

Image Generation Astrophysics of Galaxies